. . "NGC 1851 \u2014 \u043A\u0443\u043B\u044C\u043E\u0432\u0435 \u0441\u043A\u0443\u043F\u0447\u0435\u043D\u043D\u044F \u0442\u0438\u043F\u0443 II \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0413\u043E\u043B\u0443\u0431. \u0412\u0456\u0434\u043A\u0440\u0438\u0432\u0430\u0447\u0435\u043C \u0446\u044C\u043E\u0433\u043E \u043E\u0431'\u0454\u043A\u0442\u0430 \u0454 \u0414\u0436\u0435\u0439\u043C\u0441 \u0414\u0430\u043D\u043B\u043E\u043F, \u044F\u043A\u0438\u0439 \u0443\u043F\u0435\u0440\u0448\u0435 \u0441\u043F\u043E\u0441\u0442\u0435\u0440\u0456\u0433\u0430\u0432 \u0437\u0430 \u043E\u0431'\u0454\u043A\u0442\u043E\u043C 10 \u0442\u0440\u0430\u0432\u043D\u044F 1826. \u0426\u0435\u0439 \u043E\u0431'\u0454\u043A\u0442 \u043C\u0456\u0441\u0442\u0438\u0442\u044C\u0441\u044F \u0432 \u043E\u0440\u0438\u0433\u0456\u043D\u0430\u043B\u044C\u043D\u0456\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0456\u0457 \u041D\u043E\u0432\u043E\u0433\u043E \u0437\u0430\u0433\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0443."@uk . . "\u0623\u0646 \u062C\u064A \u0633\u064A 1851 (NGC 1851\u060C \u0627\u0644\u0645\u0639\u0631\u0648\u0641 \u0623\u064A\u0636\u0627 \u0628\u0627\u0633\u0645 \u0643\u0627\u0644\u062F\u0648\u064A\u0644 73) \u0647\u0648 \u0639\u0646\u0642\u0648\u062F \u0645\u063A\u0644\u0642 \u0648 \u0647\u0648 \u0639\u0646\u0642\u0648\u062F \u0636\u062E\u0645 \u0646\u0633\u0628\u064A\u0627\u064B \u064A\u0642\u0639 \u0641\u064A \u062C\u0646\u0648\u0628 \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u062D\u0645\u0627\u0645\u0629. \u0648\u0635\u0641\u0647 \u0639\u0627\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u062C\u0648\u0646 \u062F\u0631\u0627\u064A\u0631 \u0628\u0623\u0646\u0647 \u0644\u064A\u0633 \u0644\u0627\u0645\u0639\u0627\u064B \u062C\u062F\u0627\u064B \u0648\u0644\u0643\u0646\u0647 \u0643\u0628\u064A\u0631 \u062C\u062F\u0627\u064B \u0648\u0645\u0633\u062A\u062F\u064A\u0631 \u0648 \u0645\u064F\u062D\u062F\u062F \u062C\u064A\u062F\u0627\u064B \u0648\u064A\u062A\u0623\u0644\u0641 \u0645\u0646 \u0646\u062C\u0648\u0645 \u0628\u0634\u0643\u0644 \u0648\u0627\u0636\u062D \u064A\u0642\u0639 \u0639\u0644\u0649 \u0628\u0639\u062F 39.5 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u0645\u0646 \u0627\u0644\u0634\u0645\u0633\u060C \u0648 54.1 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u0645\u0646 \u0645\u0631\u0643\u0632 \u0627\u0644\u0645\u062C\u0631\u0629 . \u064A\u0633\u064A\u0631 \u0627\u0644\u0639\u0646\u0642\u0648\u062F \u0641\u064A \u0645\u062F\u0627\u0631 \u0634\u062F\u064A\u062F \u0627\u0644\u0625\u0646\u062D\u0631\u0627\u0641 \u0639\u0628\u0631 \u0627\u0644\u0645\u062C\u0631\u0629\u060C \u0645\u0639 \u0625\u0646\u062D\u0631\u0627\u0641 \u064A\u0628\u0644\u063A \u062D\u0648\u0627\u0644\u064A 0.7"@ar . "73"^^ . "NGC 1851 es un c\u00FAmulo globular ubicado en la constelaci\u00F3n de Columba, la Paloma. Se lo conoce tambi\u00E9n como Caldwell 73. Su magnitud aparente es de 7.3Est\u00E1 a 39,500 al,\u200B y se ubica a unos 8\u00B0 al sudoeste de la estrella de magnitud 2.65 Phact (\u03B1 Columbae)."@es . "\u0623\u0646 \u062C\u064A \u0633\u064A 1851 (NGC 1851\u060C \u0627\u0644\u0645\u0639\u0631\u0648\u0641 \u0623\u064A\u0636\u0627 \u0628\u0627\u0633\u0645 \u0643\u0627\u0644\u062F\u0648\u064A\u0644 73) \u0647\u0648 \u0639\u0646\u0642\u0648\u062F \u0645\u063A\u0644\u0642 \u0648 \u0647\u0648 \u0639\u0646\u0642\u0648\u062F \u0636\u062E\u0645 \u0646\u0633\u0628\u064A\u0627\u064B \u064A\u0642\u0639 \u0641\u064A \u062C\u0646\u0648\u0628 \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u062D\u0645\u0627\u0645\u0629. \u0648\u0635\u0641\u0647 \u0639\u0627\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u062C\u0648\u0646 \u062F\u0631\u0627\u064A\u0631 \u0628\u0623\u0646\u0647 \u0644\u064A\u0633 \u0644\u0627\u0645\u0639\u0627\u064B \u062C\u062F\u0627\u064B \u0648\u0644\u0643\u0646\u0647 \u0643\u0628\u064A\u0631 \u062C\u062F\u0627\u064B \u0648\u0645\u0633\u062A\u062F\u064A\u0631 \u0648 \u0645\u064F\u062D\u062F\u062F \u062C\u064A\u062F\u0627\u064B \u0648\u064A\u062A\u0623\u0644\u0641 \u0645\u0646 \u0646\u062C\u0648\u0645 \u0628\u0634\u0643\u0644 \u0648\u0627\u0636\u062D \u064A\u0642\u0639 \u0639\u0644\u0649 \u0628\u0639\u062F 39.5 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u0645\u0646 \u0627\u0644\u0634\u0645\u0633\u060C \u0648 54.1 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u0645\u0646 \u0645\u0631\u0643\u0632 \u0627\u0644\u0645\u062C\u0631\u0629 . \u064A\u0633\u064A\u0631 \u0627\u0644\u0639\u0646\u0642\u0648\u062F \u0641\u064A \u0645\u062F\u0627\u0631 \u0634\u062F\u064A\u062F \u0627\u0644\u0625\u0646\u062D\u0631\u0627\u0641 \u0639\u0628\u0631 \u0627\u0644\u0645\u062C\u0631\u0629\u060C \u0645\u0639 \u0625\u0646\u062D\u0631\u0627\u0641 \u064A\u0628\u0644\u063A \u062D\u0648\u0627\u0644\u064A 0.7"@ar . . "NGC 1851 (Caldwell 73) est un amas globulaire situ\u00E9 dans la constellation de la Colombe. Il a \u00E9t\u00E9 d\u00E9couvert par l'astronome \u00E9cossais James Dunlop en 1826. \n* NGC 1851 en ultraviolet par le t\u00E9lescope spatial GALEX. \n* NGC 1851 par le t\u00E9lescope spatial Hubble. Selon une \u00E9tude publi\u00E9e en 2011 par J. Boyles et ses coll\u00E8gues, la m\u00E9tallicit\u00E9 de l'amas NGC 1851 est \u00E9gale \u00E0 -1,18 et sa masse est \u00E9gale \u00E0 551 000. Dans cette m\u00EAme \u00E9tude, la distance de l'amas est estim\u00E9e \u00E0 environ 12,1 kpc (\u223C39 500 a.l.)."@fr . "NGC 1851\uFF08\u4E5F\u7A31\u70BACaldwell 73\uFF09\u4F4D\u65BC\u5929\u9D3F\u5EA7\u7684\u5357\u90E8\uFF0C\u662F\u4E00\u500B\u76F8\u5C0D\u5DE8\u5927\u7684\u7403\u72C0\u661F\u5718\u3002\u5929\u6587\u5B78\u5BB6\u8A79\u59C6\u58EB\u00B7\u6566\u6D1B\u666E\u63CF\u8FF0\u5B83\u4E0D\u662F\u975E\u5E38\u660E\u4EAE\uFF0C\u4F46\u975E\u5E38\u5927\uFF0C\u5713\u5F62\uFF0C\u5206\u8FA8\u7387\u5F88\u597D\uFF0C\u660E\u986F\u7531\u6046\u661F\u7D44\u6210\u3002\u5B83\u8DDD\u96E2\u592A\u967D 39.5\u5343\u5149\u5E74\uFF0C\u8DDD\u96E2\u9280\u6CB3\u4E2D\u5FC3 54.1\u5343\u5149\u5E74\u3002\u661F\u5718\u6CBF\u8457\u4E00\u500B\u9AD8\u5EA6\u504F\u5FC3\u7684\u8ECC\u9053\u7A7F\u904E\u9280\u6CB3\u7CFB\uFF0C\u5176\u96E2\u5FC3\u7387\u7D04\u70BA0.7\u3002 \u9019\u500B\u7269\u9AD4\u5728\u590F\u666E\u529B-\u7D22\u8036\u96C6\u4E2D\u5EA6\u5206\u985E\u6CD5\u4E2D\u5C6C\u65BCII\uFF0C\u986F\u793A\u6046\u661F\u5BC6\u96C6\u7684\u5411\u4E2D\u5FC3\u96C6\u4E2D\u3002\u5B83\u662F\u5DF2\u77E5\u7684\u9280\u6CB3\u7403\u72C0\u661F\u5718\u4E2D\u5BC6\u5EA6\u6700\u9AD8\u7684\u661F\u5718\u4E4B\u4E00\u3002\u6046\u661F\u6210\u5206\u986F\u793A\u4E86\u5169\u500B\u7368\u7ACB\u7684\u6B21\u5DE8\u661F\u7FA4\u9AD4\uFF0C\u8F03\u4EAE\u7684\u5206\u652F\u66F4\u96C6\u4E2D\u5728\u661F\u5718\u7684\u5916\u90E8\u5340\u57DF\u3002\u4F30\u8A08NGC 1851\u7684\u5E74\u9F61\u7D04\u70BA92\u5104\u5E74\uFF0C\u8CEA\u91CF\u70BA\u592A\u967D\u7684551,000\u500D\u3002 \u661F\u5718\u5468\u570D\u662F\u4E00\u500B\u6F2B\u5C04\u7684\u6046\u661F\u6688\uFF0C\u5411\u5916\u5EF6\u4F38\u5230{}{Val | 240 | u=pc}\u6216\u66F4\u5927\u7684\u534A\u5F91\u3002\u9019\u4E00\u7279\u5FB5\uFF0C\u5982\u679C\u518D\u52A0\u4E0A\u7F3A\u4E4F\u6F6E\u6C50\u5C3E\u6216\u76F8\u95DC\u7684\u661F\u6D41\uFF0C\u8868\u660E\u661F\u5718\u53EF\u80FD\u662F\u4E00\u500B\u525D\u96E2\u7684\u77EE\u661F\u7CFB\u6838\uFF0C\u985E\u4F3C\u65BC\u88AB\u9280\u6CB3\u7CFB\u5438\u7A4D\u534A\u4EBA\u99AC\u5EA7\u03C9\uFF1B\u4F46\u662F\u6F6E\u6C50\u5C3E\u4ECD\u7136\u5B58\u5728\u3002 \u8A72\u661F\u5718\u4E5F\u53EF\u80FD\u662F\u5169\u500B\u7368\u7ACB\u661F\u5718\u5408\u4F75\u7684\u7D50\u679C\uFF0C\u4F46\u5B83\u5011\u9700\u8981\u5177\u6709\u76F8\u540C\u7684\u91D1\u5C6C\u8C50\u5EA6\uFF08\u5929\u6587\u5B78\u5BB6\u6240\u8B02\u7A31\u6C2B\u548C\u6C26\u4E4B\u5916\u7684\u5143\u7D20\u8C50\u5EA6\uFF09\u3002\u9019\u4E00\u4E8B\u5BE6\u4F7F\u5F97\u9019\u7A2E\u60C5\u6CC1\u4E0D\u592A\u53EF\u80FD\u767C\u751F\u3002"@zh . "7.3"^^ . "NGC 1851"@uk . . "NGC 1851 (aliaj indikoj \u2014 GCL 9, ESO 305-SC16) estas globa stelamaso en konstelacio Kolombo. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo."@eo . . "NGC 1851"@pt . . . . . "NGC 1851"@en . . . . "NGC 1851"@it . . . . . . "NGC 1851"@nl . . . "NGC 1851 (r\u00F3wnie\u017C GCL 9 lub ESO 305-SC16) \u2013 gromada kulista, znajduj\u0105ca si\u0119 w gwiazdozbiorze Go\u0142\u0119bia. Jest oddalona o oko\u0142o 39,5 tys. lat \u015Bwietlnych od S\u0142o\u0144ca i o 54,1 tys. lat \u015Bwietlnych od centrum Galaktyki. Odkry\u0142 j\u0105 James Dunlop 10 maja 1826. W roku 2003 odkryto, \u017Ce NGC 1851 mo\u017Ce pochodzi\u0107 z galaktyki Karze\u0142 Wielkiego Psa. Opr\u00F3cz NGC 1851 podobne pochodzenie mia\u0142yby mie\u0107 obiekty Messier 79, NGC 2298 i NGC 2808."@pl . "NGC 1851 izar kumulu bat da, Columba konstelazioan. aurkitu zuen 1826ko maiatzaren\u202F10an."@eu . . "NGC 1851 (tak\u00E9 zn\u00E1m\u00E1 jako Caldwell 73) je jasn\u00E1 kulov\u00E1 hv\u011Bzdokupa v souhv\u011Bzd\u00ED Holubice nach\u00E1zej\u00EDc\u00ED se ve vzd\u00E1lenosti 39 400 sv\u011Bteln\u00FDch let od Zem\u011B. Objevil ji 29. kv\u011Btna 1826 australsk\u00FD astronom James Dunlop."@cs . "NGC 1851, \u00E4ven k\u00E4nd som Caldwell 73, \u00E4r en klotformig stj\u00E4rnhop i stj\u00E4rnbild Duvan. Hopen uppt\u00E4cktes i 1826 av den skotske atronomen James Dunlop, som beskrev den som \"inte s\u00E4rskilt ljus men mycket stor, rund, v\u00E4l uppl\u00F6st och tydligt best\u00E5ende av stj\u00E4rnor\". Den \u00E4r bel\u00E4gen 39 500 ljus\u00E5r fr\u00E5n solen, och 54 100 ljus\u00E5r fr\u00E5n Vintergatans centrum. Hopen f\u00F6ljer en mycket excentrisk bana genom galaxen, med en excentricitet p\u00E5 ca 0,7."@sv . "NGC 1851 ist die Bezeichnung eines Kugelsternhaufens im Sternbild Columba. NGC 1851 hat einen Durchmesser von 12 Bogenminuten. Dieser Haufen, der nur von S\u00FCdeuropa oder s\u00FCdlicheren Breiten sichtbar ist, ist einer der wenigen Kugelsternhaufen am Winterhimmel. Diese Tatsache erhielt zus\u00E4tzliche Brisanz durch die Entdeckung der Canis-Major-Zwerggalaxie im Jahre 2003. Genau wie Messier 79 und NGC 2808 scheint dieser Sternhaufen seinen Ursprung nicht im Milchstra\u00DFensystem zu haben, sondern wurde zusammen mit jener Zwerggalaxie eingefangen. \n*"@de . . . . . . . "To NGC 1851 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C3\u03C6\u03B1\u03B9\u03C1\u03C9\u03C4\u03CC \u03C3\u03BC\u03AE\u03BD\u03BF\u03C2 \u03C3\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u03A0\u03B5\u03C1\u03B9\u03C3\u03C4\u03B5\u03C1\u03AC. \u0391\u03C0\u03AD\u03C7\u03B5\u03B9 \u03B1\u03C0\u03CC \u03C4\u03B7 \u0393\u03B7 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 39.800 \u03AD\u03C4\u03B7 \u03C6\u03C9\u03C4\u03CC\u03C2, \u03CC\u03C0\u03C9\u03C2 \u03C5\u03C0\u03BF\u03BB\u03BF\u03B3\u03AF\u03C3\u03C4\u03B7\u03BA\u03B5 \u03B1\u03C0\u03CC \u03C4\u03B7\u03BD \u03BC\u03B5\u03BB\u03AD\u03C4\u03B7 \u03C4\u03C9\u03BD \u03BC\u03B5\u03C4\u03B1\u03B2\u03BB\u03B7\u03C4\u03CE\u03BD \u03C4\u03CD\u03C0\u03BF\u03C5 RR \u039B\u03CD\u03C1\u03B1\u03C2, \u03BA\u03B1\u03B9 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 54.000 \u03AD\u03C4\u03B7 \u03C6\u03C9\u03C4\u03CC\u03C2 \u03B1\u03C0\u03CC \u03C4\u03BF \u03BA\u03AD\u03BD\u03C4\u03C1\u03BF \u03C4\u03BF\u03C5 \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1. \u03A0\u03B9\u03B8\u03B1\u03BD\u03CC\u03BD \u03BD\u03B1 \u03AE\u03C4\u03B1\u03BD \u03C4\u03BC\u03AE\u03BC\u03B1 \u03C4\u03BF\u03C5 \u03BD\u03AC\u03BD\u03BF\u03C5 \u03C4\u03BF\u03C5 \u039C\u03B5\u03B3\u03AC\u03BB\u03BF\u03C5 \u039A\u03C5\u03BD\u03CC\u03C2, \u03B5\u03BD\u03CC\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BD\u03AC\u03BD\u03BF\u03C5 \u03BF \u03BF\u03C0\u03BF\u03AF\u03BF\u03C2 \u03B2\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03C3\u03B5 \u03B4\u03B9\u03B1\u03B4\u03B9\u03BA\u03B1\u03C3\u03AF\u03B1 \u03C3\u03C5\u03B3\u03C7\u03CE\u03BD\u03B5\u03C5\u03C3\u03B7\u03C2 \u03BC\u03B5 \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1. \u039C\u03B1\u03B6\u03AF \u03BC\u03B5 \u03C4\u03BF NGC 1851, \u03AC\u03BB\u03BB\u03B1 \u03C4\u03C1\u03AF\u03B1 \u03C3\u03C6\u03B1\u03B9\u03C1\u03C9\u03C4\u03AC \u03C3\u03BC\u03AE\u03BD\u03B7 \u03C0\u03B9\u03B8\u03B1\u03BD\u03CE\u03C2 \u03B1\u03BD\u03AE\u03BA\u03BF\u03C5\u03BD \u03C3\u03C4\u03BF \u03BD\u03AC\u03BD\u03BF \u03C4\u03BF\u03C5 \u039C\u03B5\u03B3\u03AC\u03BB\u03BF\u03C5 \u039A\u03C5\u03BD\u03CC\u03C2, \u03C4\u03BF \u039C\u03B5\u03C3\u03B9\u03AD 79, \u03C4\u03BF NGC 2298 \u03BA\u03B1\u03B9 \u03C4\u03BF . \u03A4\u03BF \u03B1\u03BD\u03B1\u03BA\u03AC\u03BB\u03C5\u03C8\u03B5 \u03BF \u03A4\u03B6\u03AD\u03B9\u03BC\u03C2 \u039D\u03C4\u03AC\u03BD\u03BB\u03BF\u03C0 \u03C4\u03B9\u03C2 29 \u039C\u03B1\u0390\u03BF\u03C5 1826. \u0388\u03C7\u03B5\u03B9 \u03C6\u03B1\u03B9\u03BD\u03CC\u03BC\u03B5\u03BD\u03BF \u03BC\u03AD\u03B3\u03B5\u03B8\u03BF\u03C2 +7,14."@el . "1851"^^ . "NGC 1851 (\u0434\u0440\u0443\u0433\u0438\u0435 \u043E\u0431\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u2014 GCL 9, ESO 305-SC16) \u2014 \u0448\u0430\u0440\u043E\u0432\u043E\u0435 \u0441\u043A\u043E\u043F\u043B\u0435\u043D\u0438\u0435 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0413\u043E\u043B\u0443\u0431\u044F. \u041D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043E\u043A\u043E\u043B\u043E 40 \u0442\u044B\u0441\u044F\u0447 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u042D\u0442\u043E\u0442 \u043E\u0431\u044A\u0435\u043A\u0442 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0447\u0438\u0441\u043B\u043E \u043F\u0435\u0440\u0435\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u044B\u0445 \u0432 \u043E\u0440\u0438\u0433\u0438\u043D\u0430\u043B\u044C\u043D\u043E\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0438\u0438 \u00AB\u041D\u043E\u0432\u043E\u0433\u043E \u043E\u0431\u0449\u0435\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0430\u00BB."@ru . . "NGC 1851"@eo . . . . . "NGC 1851 (r\u00F3wnie\u017C GCL 9 lub ESO 305-SC16) \u2013 gromada kulista, znajduj\u0105ca si\u0119 w gwiazdozbiorze Go\u0142\u0119bia. Jest oddalona o oko\u0142o 39,5 tys. lat \u015Bwietlnych od S\u0142o\u0144ca i o 54,1 tys. lat \u015Bwietlnych od centrum Galaktyki. Odkry\u0142 j\u0105 James Dunlop 10 maja 1826. W roku 2003 odkryto, \u017Ce NGC 1851 mo\u017Ce pochodzi\u0107 z galaktyki Karze\u0142 Wielkiego Psa. Opr\u00F3cz NGC 1851 podobne pochodzenie mia\u0142yby mie\u0107 obiekty Messier 79, NGC 2298 i NGC 2808."@pl . . "NGC 1851"@ar . . "GCl 9, ESO 305-SC 016, Caldwell 73, Melotte 30"@en . . . . "NGC 1851 (Caldwell 73) est un amas globulaire situ\u00E9 dans la constellation de la Colombe. Il a \u00E9t\u00E9 d\u00E9couvert par l'astronome \u00E9cossais James Dunlop en 1826. \n* NGC 1851 en ultraviolet par le t\u00E9lescope spatial GALEX. \n* NGC 1851 par le t\u00E9lescope spatial Hubble. Selon une \u00E9tude publi\u00E9e en 2011 par J. Boyles et ses coll\u00E8gues, la m\u00E9tallicit\u00E9 de l'amas NGC 1851 est \u00E9gale \u00E0 -1,18 et sa masse est \u00E9gale \u00E0 551 000. Dans cette m\u00EAme \u00E9tude, la distance de l'amas est estim\u00E9e \u00E0 environ 12,1 kpc (\u223C39 500 a.l.). Selon une autre \u00E9tude publi\u00E9e en 2010, la m\u00E9tallicit\u00E9 de NGC 1851 est estim\u00E9e \u00E0 -1,03 [Fe/H] et son \u00E2ge \u00E0 9,98 milliards d'ann\u00E9es."@fr . . "NGC 1851 \u00E9s un c\u00FAmul globular situat en la constel\u00B7laci\u00F3 de Coloma."@ca . . "11250228"^^ . . "\u22127.80"@en . . . "NGC 1851 \u00E9 um aglomerado globular classe II localizado na constela\u00E7\u00E3o de Columba. Foi descoberto em 1826 pelo astr\u00F4nomo brit\u00E2nico James Dunlop. Juntamente com NGC 1904, NGC2298 e NGC 2808, acredita-se que tenha feito parte do sistema de aglomerados globulares da Gal\u00E1xia An\u00E3 do C\u00E3o Maior no passado, antes desta ter sido acrescida \u00E0 Via L\u00E1ctea."@pt . . . "NGC 1851"@ca . . "NGC 1851 (\u0434\u0440\u0443\u0433\u0438\u0435 \u043E\u0431\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u2014 GCL 9, ESO 305-SC16) \u2014 \u0448\u0430\u0440\u043E\u0432\u043E\u0435 \u0441\u043A\u043E\u043F\u043B\u0435\u043D\u0438\u0435 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0413\u043E\u043B\u0443\u0431\u044F. \u041D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043E\u043A\u043E\u043B\u043E 40 \u0442\u044B\u0441\u044F\u0447 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u042D\u0442\u043E\u0442 \u043E\u0431\u044A\u0435\u043A\u0442 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0447\u0438\u0441\u043B\u043E \u043F\u0435\u0440\u0435\u0447\u0438\u0441\u043B\u0435\u043D\u043D\u044B\u0445 \u0432 \u043E\u0440\u0438\u0433\u0438\u043D\u0430\u043B\u044C\u043D\u043E\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0438\u0438 \u00AB\u041D\u043E\u0432\u043E\u0433\u043E \u043E\u0431\u0449\u0435\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0430\u00BB."@ru . "An Ultraviolet image of NGC 1851."@en . . . . . "11"^^ . . . . . . "NGC 1851"@ru . "NGC 1851 (noto anche come C 73) \u00E8 un ammasso globulare visibile nella costellazione della Colomba. Visibile appena con un binocolo, un telescopio di 150mm di apertura gi\u00E0 inizia a mostrare le componenti pi\u00F9 brillanti; tuttavia il centro dell'ammasso, esteso su 5' d'arco, \u00E8 estremamente concentrato, al punto che diventa impossibile risolverlo neppure con i pi\u00F9 potenti telescopi amatoriali e semiprofessionali. NGC 1851 ha una magnitudine assoluta di -8,25, e dista dal Sole quasi 40.000 anni-luce. NGC 1851 fa parte della Salsiccia di Gaia, una galassia nana fusasi con la Via lattea circa 8, 11 miliardi di anni fa. NGC 1851 all'ultravioletto (NASA/GALEX)"@it . . . "\u22121.27"@en . . "NGC 1851\uFF08Caldwell 73\u3001Melotte 30\uFF09\u306F\u3001\u306F\u3068\u5EA7\u306B\u3042\u308B\u7403\u72B6\u661F\u56E3\u3067\u3042\u308B\u3002"@ja . . . "9.199999999999999"^^ . . . . . . "NGC 1851"@fr . "NGC 1851 \u00E9 um aglomerado globular classe II localizado na constela\u00E7\u00E3o de Columba. Foi descoberto em 1826 pelo astr\u00F4nomo brit\u00E2nico James Dunlop. Juntamente com NGC 1904, NGC2298 e NGC 2808, acredita-se que tenha feito parte do sistema de aglomerados globulares da Gal\u00E1xia An\u00E3 do C\u00E3o Maior no passado, antes desta ter sido acrescida \u00E0 Via L\u00E1ctea."@pt . "NGC 1851"@pl . "NGC 1851 \u00E9s un c\u00FAmul globular situat en la constel\u00B7laci\u00F3 de Coloma."@ca . . . "NGC 1851\uFF08\u4E5F\u7A31\u70BACaldwell 73\uFF09\u4F4D\u65BC\u5929\u9D3F\u5EA7\u7684\u5357\u90E8\uFF0C\u662F\u4E00\u500B\u76F8\u5C0D\u5DE8\u5927\u7684\u7403\u72C0\u661F\u5718\u3002\u5929\u6587\u5B78\u5BB6\u8A79\u59C6\u58EB\u00B7\u6566\u6D1B\u666E\u63CF\u8FF0\u5B83\u4E0D\u662F\u975E\u5E38\u660E\u4EAE\uFF0C\u4F46\u975E\u5E38\u5927\uFF0C\u5713\u5F62\uFF0C\u5206\u8FA8\u7387\u5F88\u597D\uFF0C\u660E\u986F\u7531\u6046\u661F\u7D44\u6210\u3002\u5B83\u8DDD\u96E2\u592A\u967D 39.5\u5343\u5149\u5E74\uFF0C\u8DDD\u96E2\u9280\u6CB3\u4E2D\u5FC3 54.1\u5343\u5149\u5E74\u3002\u661F\u5718\u6CBF\u8457\u4E00\u500B\u9AD8\u5EA6\u504F\u5FC3\u7684\u8ECC\u9053\u7A7F\u904E\u9280\u6CB3\u7CFB\uFF0C\u5176\u96E2\u5FC3\u7387\u7D04\u70BA0.7\u3002 \u9019\u500B\u7269\u9AD4\u5728\u590F\u666E\u529B-\u7D22\u8036\u96C6\u4E2D\u5EA6\u5206\u985E\u6CD5\u4E2D\u5C6C\u65BCII\uFF0C\u986F\u793A\u6046\u661F\u5BC6\u96C6\u7684\u5411\u4E2D\u5FC3\u96C6\u4E2D\u3002\u5B83\u662F\u5DF2\u77E5\u7684\u9280\u6CB3\u7403\u72C0\u661F\u5718\u4E2D\u5BC6\u5EA6\u6700\u9AD8\u7684\u661F\u5718\u4E4B\u4E00\u3002\u6046\u661F\u6210\u5206\u986F\u793A\u4E86\u5169\u500B\u7368\u7ACB\u7684\u6B21\u5DE8\u661F\u7FA4\u9AD4\uFF0C\u8F03\u4EAE\u7684\u5206\u652F\u66F4\u96C6\u4E2D\u5728\u661F\u5718\u7684\u5916\u90E8\u5340\u57DF\u3002\u4F30\u8A08NGC 1851\u7684\u5E74\u9F61\u7D04\u70BA92\u5104\u5E74\uFF0C\u8CEA\u91CF\u70BA\u592A\u967D\u7684551,000\u500D\u3002 \u661F\u5718\u5468\u570D\u662F\u4E00\u500B\u6F2B\u5C04\u7684\u6046\u661F\u6688\uFF0C\u5411\u5916\u5EF6\u4F38\u5230{}{Val | 240 | u=pc}\u6216\u66F4\u5927\u7684\u534A\u5F91\u3002\u9019\u4E00\u7279\u5FB5\uFF0C\u5982\u679C\u518D\u52A0\u4E0A\u7F3A\u4E4F\u6F6E\u6C50\u5C3E\u6216\u76F8\u95DC\u7684\u661F\u6D41\uFF0C\u8868\u660E\u661F\u5718\u53EF\u80FD\u662F\u4E00\u500B\u525D\u96E2\u7684\u77EE\u661F\u7CFB\u6838\uFF0C\u985E\u4F3C\u65BC\u88AB\u9280\u6CB3\u7CFB\u5438\u7A4D\u534A\u4EBA\u99AC\u5EA7\u03C9\uFF1B\u4F46\u662F\u6F6E\u6C50\u5C3E\u4ECD\u7136\u5B58\u5728\u3002 \u8A72\u661F\u5718\u4E5F\u53EF\u80FD\u662F\u5169\u500B\u7368\u7ACB\u661F\u5718\u5408\u4F75\u7684\u7D50\u679C\uFF0C\u4F46\u5B83\u5011\u9700\u8981\u5177\u6709\u76F8\u540C\u7684\u91D1\u5C6C\u8C50\u5EA6\uFF08\u5929\u6587\u5B78\u5BB6\u6240\u8B02\u7A31\u6C2B\u548C\u6C26\u4E4B\u5916\u7684\u5143\u7D20\u8C50\u5EA6\uFF09\u3002\u9019\u4E00\u4E8B\u5BE6\u4F7F\u5F97\u9019\u7A2E\u60C5\u6CC1\u4E0D\u592A\u53EF\u80FD\u767C\u751F\u3002 PSR J0514-4002A\u662FNGC 1851\u4E2D\u7684\u6BEB\u79D2\u8108\u885D\u661F\uFF0C\u5B83\u6B63\u570D\u7E5E\u8457\u4E00\u9846\u53EF\u80FD\u4E5F\u662F\u4E2D\u5B50\u661F\u7684\u5927\u8CEA\u91CF\u5929\u9AD4\u904B\u884C\u3002\u9019\u4E00\u5C0D\u7684\u8ECC\u9053\u9031\u671F\u70BA18.8\u65E5\uFF0C\u96E2\u5FC3\u7387\u70BA0.89\u3002\u5728\u661F\u5718\u4E2D\u5DF2\u7D93\u767C\u73FE\u4E8643\u9846\u5929\u7434\u5EA7RR\u578B\u8B8A\u661F\uFF0C\u9019\u8868\u660E\u9019\u662F\u4E00\u500BOosterhoff I\u578B\u661F\u5718\uFF0C\u4F46\u5176\u6027\u8CEA\u8207II\u578B\u76F8\u4F3C\u3002\u5DF2\u7D93\u89C0\u5BDF\u5230\u5169\u7A2E\u6C34\u5E73\u5206\u652F\u661F\u7684\u7A2E\u7FA4\uFF0C\u5176\u5E74\u9F61\u76F8\u5DEE\u7D0420\u5104\u5E74\u3002\u5C0D\u7D05\u5DE8\u661F\u5206\u652F\u6210\u54E1\u6052\u661F\u7684\u5149\u8B5C\u5206\u6790\u8868\u660E\uFF0C\u661F\u5718\u4E2D\u5BE6\u969B\u4E0A\u6709\u4E09\u7A2E\u4E0D\u540C\u7684\u6052\u661F\u7FA4\u3002"@zh . "NGC 1851"@el . . . . . "NGC 1851 (also known as Caldwell 73) is a relatively massive globular cluster located in the southern constellation of Columba. Astronomer John Dreyer described it as not very bright but very large, round, well resolved, and clearly consisting of stars. It is located 39.5 kilolight-years from the Sun, and 54.1 kilolight-years from the Galactic Center. The cluster is following a highly eccentric orbit through the galaxy, with an eccentricity of about 0.7 This object has a Shapley\u2013Sawyer Concentration Class of II, indicating a dense central concentration. It has one of the highest concentrations known for Galactic globular clusters. The stellar components shows two separate populations of subgiant stars, with the brighter branch being more concentrated in the outer regions of the cluster. NGC 1851 is an estimated 9.2 billion years old with 551,000 times the mass of the Sun. The cluster is surrounded by a diffuse halo of stars that stretches outward to a radius of 240 pc or more. This feature, if combined with the lack of tidal tail or associated stream of stars, suggests the cluster may be a stripped dwarf galaxy nuclei, similar to Omega Centauri, that has been accreted by the Milky Way. The tidal tail is still present though. It is also possible the cluster is the result of the merger of two separate clusters, but the fact that they would need to have the same metallicity \u2013 what astronomers term the abundance of elements other than hydrogen and helium \u2013 makes this scenario less likely. PSR J0514-4002A is a milli-second pulsar in NGC 1851. It is orbiting a massive object that may also be a neutron star. The pair have an orbital period of 18.8 days with a large eccentricity of 0.89. 43 RR Lyrae variables have been discovered in the cluster, which show this to be an Oosterhoff type I cluster but having properties similar to type II. Two populations of horizontal branch stars have been observed, with the pair having an age difference of around two billion years. Spectroscopic analysis of the red giant branch member stars suggests there are actually three different populations of stars in the cluster."@en . . . . . . "NGC 1851"@sv . . . . "NGC 1851"@ja . "NGC 1851 ist die Bezeichnung eines Kugelsternhaufens im Sternbild Columba. NGC 1851 hat einen Durchmesser von 12 Bogenminuten. Dieser Haufen, der nur von S\u00FCdeuropa oder s\u00FCdlicheren Breiten sichtbar ist, ist einer der wenigen Kugelsternhaufen am Winterhimmel. Diese Tatsache erhielt zus\u00E4tzliche Brisanz durch die Entdeckung der Canis-Major-Zwerggalaxie im Jahre 2003. Genau wie Messier 79 und NGC 2808 scheint dieser Sternhaufen seinen Ursprung nicht im Milchstra\u00DFensystem zu haben, sondern wurde zusammen mit jener Zwerggalaxie eingefangen. Das Objekt wurde im Jahr 1826 von dem schottischen Astronomen James Dunlop entdeckt. \n* Ultraviolettfotografie von NGC 1851, aufgenommen von GALEX"@de . . "NGC 1851 \u2014 \u043A\u0443\u043B\u044C\u043E\u0432\u0435 \u0441\u043A\u0443\u043F\u0447\u0435\u043D\u043D\u044F \u0442\u0438\u043F\u0443 II \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0413\u043E\u043B\u0443\u0431. \u0412\u0456\u0434\u043A\u0440\u0438\u0432\u0430\u0447\u0435\u043C \u0446\u044C\u043E\u0433\u043E \u043E\u0431'\u0454\u043A\u0442\u0430 \u0454 \u0414\u0436\u0435\u0439\u043C\u0441 \u0414\u0430\u043D\u043B\u043E\u043F, \u044F\u043A\u0438\u0439 \u0443\u043F\u0435\u0440\u0448\u0435 \u0441\u043F\u043E\u0441\u0442\u0435\u0440\u0456\u0433\u0430\u0432 \u0437\u0430 \u043E\u0431'\u0454\u043A\u0442\u043E\u043C 10 \u0442\u0440\u0430\u0432\u043D\u044F 1826. \u0426\u0435\u0439 \u043E\u0431'\u0454\u043A\u0442 \u043C\u0456\u0441\u0442\u0438\u0442\u044C\u0441\u044F \u0432 \u043E\u0440\u0438\u0433\u0456\u043D\u0430\u043B\u044C\u043D\u0456\u0439 \u0440\u0435\u0434\u0430\u043A\u0446\u0456\u0457 \u041D\u043E\u0432\u043E\u0433\u043E \u0437\u0430\u0433\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u0430\u0442\u0430\u043B\u043E\u0433\u0443."@uk . "NGC 1851\uFF08Caldwell 73\u3001Melotte 30\uFF09\u306F\u3001\u306F\u3068\u5EA7\u306B\u3042\u308B\u7403\u72B6\u661F\u56E3\u3067\u3042\u308B\u3002"@ja . . "NGC 1851 (tak\u00E9 zn\u00E1m\u00E1 jako Caldwell 73) je jasn\u00E1 kulov\u00E1 hv\u011Bzdokupa v souhv\u011Bzd\u00ED Holubice nach\u00E1zej\u00EDc\u00ED se ve vzd\u00E1lenosti 39 400 sv\u011Bteln\u00FDch let od Zem\u011B. Objevil ji 29. kv\u011Btna 1826 australsk\u00FD astronom James Dunlop."@cs . . . . . . . "NGC 1851 (also known as Caldwell 73) is a relatively massive globular cluster located in the southern constellation of Columba. Astronomer John Dreyer described it as not very bright but very large, round, well resolved, and clearly consisting of stars. It is located 39.5 kilolight-years from the Sun, and 54.1 kilolight-years from the Galactic Center. The cluster is following a highly eccentric orbit through the galaxy, with an eccentricity of about 0.7"@en . . "NGC 1851 is een bolvormige sterrenhoop in het sterrenbeeld Duif. Het hemelobject ligt 39.500 lichtjaar van de Aarde verwijderd en werd op 10 mei 1826 ontdekt door de Schotse astronoom James Dunlop."@nl . . "1050909123"^^ . "NGC 1851"@es . "NGC 1851 is een bolvormige sterrenhoop in het sterrenbeeld Duif. Het hemelobject ligt 39.500 lichtjaar van de Aarde verwijderd en werd op 10 mei 1826 ontdekt door de Schotse astronoom James Dunlop."@nl . . "NGC 1851"@cs . "NGC 1851"@eu . . . . . . . "NGC 1851, \u00E4ven k\u00E4nd som Caldwell 73, \u00E4r en klotformig stj\u00E4rnhop i stj\u00E4rnbild Duvan. Hopen uppt\u00E4cktes i 1826 av den skotske atronomen James Dunlop, som beskrev den som \"inte s\u00E4rskilt ljus men mycket stor, rund, v\u00E4l uppl\u00F6st och tydligt best\u00E5ende av stj\u00E4rnor\". Den \u00E4r bel\u00E4gen 39 500 ljus\u00E5r fr\u00E5n solen, och 54 100 ljus\u00E5r fr\u00E5n Vintergatans centrum. Hopen f\u00F6ljer en mycket excentrisk bana genom galaxen, med en excentricitet p\u00E5 ca 0,7."@sv . . . . "10641"^^ . . "II"@en . . . "NGC 1851 (aliaj indikoj \u2014 GCL 9, ESO 305-SC16) estas globa stelamaso en konstelacio Kolombo. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo."@eo . "To NGC 1851 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C3\u03C6\u03B1\u03B9\u03C1\u03C9\u03C4\u03CC \u03C3\u03BC\u03AE\u03BD\u03BF\u03C2 \u03C3\u03C4\u03BF\u03BD \u03B1\u03C3\u03C4\u03B5\u03C1\u03B9\u03C3\u03BC\u03CC \u03A0\u03B5\u03C1\u03B9\u03C3\u03C4\u03B5\u03C1\u03AC. \u0391\u03C0\u03AD\u03C7\u03B5\u03B9 \u03B1\u03C0\u03CC \u03C4\u03B7 \u0393\u03B7 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 39.800 \u03AD\u03C4\u03B7 \u03C6\u03C9\u03C4\u03CC\u03C2, \u03CC\u03C0\u03C9\u03C2 \u03C5\u03C0\u03BF\u03BB\u03BF\u03B3\u03AF\u03C3\u03C4\u03B7\u03BA\u03B5 \u03B1\u03C0\u03CC \u03C4\u03B7\u03BD \u03BC\u03B5\u03BB\u03AD\u03C4\u03B7 \u03C4\u03C9\u03BD \u03BC\u03B5\u03C4\u03B1\u03B2\u03BB\u03B7\u03C4\u03CE\u03BD \u03C4\u03CD\u03C0\u03BF\u03C5 RR \u039B\u03CD\u03C1\u03B1\u03C2, \u03BA\u03B1\u03B9 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 54.000 \u03AD\u03C4\u03B7 \u03C6\u03C9\u03C4\u03CC\u03C2 \u03B1\u03C0\u03CC \u03C4\u03BF \u03BA\u03AD\u03BD\u03C4\u03C1\u03BF \u03C4\u03BF\u03C5 \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1. \u03A0\u03B9\u03B8\u03B1\u03BD\u03CC\u03BD \u03BD\u03B1 \u03AE\u03C4\u03B1\u03BD \u03C4\u03BC\u03AE\u03BC\u03B1 \u03C4\u03BF\u03C5 \u03BD\u03AC\u03BD\u03BF\u03C5 \u03C4\u03BF\u03C5 \u039C\u03B5\u03B3\u03AC\u03BB\u03BF\u03C5 \u039A\u03C5\u03BD\u03CC\u03C2, \u03B5\u03BD\u03CC\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BD\u03AC\u03BD\u03BF\u03C5 \u03BF \u03BF\u03C0\u03BF\u03AF\u03BF\u03C2 \u03B2\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03C3\u03B5 \u03B4\u03B9\u03B1\u03B4\u03B9\u03BA\u03B1\u03C3\u03AF\u03B1 \u03C3\u03C5\u03B3\u03C7\u03CE\u03BD\u03B5\u03C5\u03C3\u03B7\u03C2 \u03BC\u03B5 \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1. \u039C\u03B1\u03B6\u03AF \u03BC\u03B5 \u03C4\u03BF NGC 1851, \u03AC\u03BB\u03BB\u03B1 \u03C4\u03C1\u03AF\u03B1 \u03C3\u03C6\u03B1\u03B9\u03C1\u03C9\u03C4\u03AC \u03C3\u03BC\u03AE\u03BD\u03B7 \u03C0\u03B9\u03B8\u03B1\u03BD\u03CE\u03C2 \u03B1\u03BD\u03AE\u03BA\u03BF\u03C5\u03BD \u03C3\u03C4\u03BF \u03BD\u03AC\u03BD\u03BF \u03C4\u03BF\u03C5 \u039C\u03B5\u03B3\u03AC\u03BB\u03BF\u03C5 \u039A\u03C5\u03BD\u03CC\u03C2, \u03C4\u03BF \u039C\u03B5\u03C3\u03B9\u03AD 79, \u03C4\u03BF NGC 2298 \u03BA\u03B1\u03B9 \u03C4\u03BF . \u03A4\u03BF \u03B1\u03BD\u03B1\u03BA\u03AC\u03BB\u03C5\u03C8\u03B5 \u03BF \u03A4\u03B6\u03AD\u03B9\u03BC\u03C2 \u039D\u03C4\u03AC\u03BD\u03BB\u03BF\u03C0 \u03C4\u03B9\u03C2 29 \u039C\u03B1\u0390\u03BF\u03C5 1826. \u0388\u03C7\u03B5\u03B9 \u03C6\u03B1\u03B9\u03BD\u03CC\u03BC\u03B5\u03BD\u03BF \u03BC\u03AD\u03B3\u03B5\u03B8\u03BF\u03C2 +7,14. \u0397 \u03B7\u03BB\u03B9\u03BA\u03AF\u03B1 \u03C4\u03BF\u03C5 \u03C5\u03C0\u03BF\u03BB\u03BF\u03B3\u03AF\u03B6\u03B5\u03C4\u03B1\u03B9 \u03C0\u03B5\u03C1\u03AF\u03C0\u03BF\u03C5 \u03C3\u03B5 14 \u03B4\u03B9\u03C2 \u03AD\u03C4\u03B7, \u03B1\u03BB\u03BB\u03AC \u03C4\u03B1 \u03AC\u03C3\u03C4\u03C1\u03B1 \u03C6\u03B1\u03AF\u03BD\u03B5\u03C4\u03B1\u03B9 \u03BD\u03B1 \u03B1\u03C0\u03BF\u03C4\u03B5\u03BB\u03BF\u03CD\u03BD\u03C4\u03B1\u03B9 \u03B1\u03C0\u03CC \u03C0\u03BB\u03B7\u03B8\u03C5\u03C3\u03BC\u03BF\u03CD\u03C2 \u03B4\u03CD\u03BF \u03B4\u03B9\u03B1\u03C6\u03BF\u03C1\u03B5\u03C4\u03B9\u03BA\u03CE\u03BD \u03B7\u03BB\u03B9\u03BA\u03B9\u03CE\u03BD, \u03BC\u03B5 \u03C4\u03B7 \u03B4\u03B9\u03B1\u03C6\u03BF\u03C1\u03AC \u03B1\u03BD\u03AC\u03BC\u03B5\u03C3\u03B1 \u03C3\u03C4\u03BF\u03C5\u03C2 \u03B4\u03CD\u03BF \u03C0\u03BB\u03B7\u03B8\u03C5\u03C3\u03BC\u03BF\u03CD\u03C2 \u03BD\u03B1 \u03B5\u03AF\u03BD\u03B1\u03B9 1 \u03B4\u03B9\u03C2 \u03AD\u03C4\u03B7, \u03BA\u03B1\u03B9 \u03C4\u03B1 \u03BC\u03AD\u03BB\u03B7 \u03C4\u03BF\u03C5 \u03C0\u03B1\u03C1\u03BF\u03C5\u03C3\u03B9\u03AC\u03B6\u03BF\u03C5\u03BD \u03BC\u03B5\u03B3\u03AC\u03BB\u03B7 \u03C0\u03BF\u03B9\u03BA\u03B9\u03BB\u03BF\u03BC\u03BF\u03C1\u03C6\u03AF\u03B1 \u03C3\u03C4\u03B7 \u03BC\u03B5\u03C4\u03B1\u03BB\u03BB\u03B9\u03BA\u03CC\u03C4\u03B7\u03C4\u03B1, \u03BA\u03B1\u03B8\u03CE\u03C2 \u03B5\u03C0\u03AF\u03C3\u03B7\u03C2 \u03BA\u03B1\u03B9 \u03C3\u03C4\u03B7 \u03C3\u03C5\u03B3\u03BA\u03AD\u03BD\u03C4\u03C1\u03C9\u03C3\u03B7 \u03B6\u03B9\u03C1\u03BA\u03BF\u03BD\u03AF\u03BF\u03C5 \u03BA\u03B1\u03B9 \u03BB\u03B1\u03BD\u03B8\u03B1\u03BD\u03AF\u03BF\u03C5. \u03A4\u03BF \u03BC\u03CC\u03BD\u03BF \u03AC\u03BB\u03BB\u03BF \u03C3\u03C6\u03B1\u03B9\u03C1\u03C9\u03C4\u03CC \u03C3\u03BC\u03AE\u03BD\u03BF\u03C2 \u03C0\u03BF\u03C5 \u03AD\u03C7\u03B5\u03B9 \u03BC\u03B5\u03BB\u03B5\u03C4\u03B7\u03B8\u03B5\u03AF \u03BA\u03B1\u03B9 \u03C0\u03B1\u03C1\u03BF\u03C5\u03C3\u03B9\u03AC\u03B6\u03B5\u03B9 \u03C0\u03B1\u03C1\u03CC\u03BC\u03BF\u03B9\u03B1 \u03C0\u03BF\u03B9\u03BA\u03B9\u03BB\u03AF\u03B1 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C4\u03BF \u03C9 \u039A\u03B5\u03BD\u03C4\u03B1\u03CD\u03C1\u03BF\u03C5, \u03AD\u03BD\u03B1 \u03B1\u03C0\u03CC \u03C4\u03B1 \u03BC\u03B5\u03B3\u03B1\u03BB\u03CD\u03C4\u03B5\u03C1\u03B1 \u03C3\u03C6\u03B1\u03B9\u03C1\u03C9\u03C4\u03AC \u03C3\u03BC\u03AE\u03BD\u03B7 \u03C4\u03BF\u03C5 \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03BA\u03B1\u03B9 \u03B8\u03B5\u03C9\u03C1\u03B5\u03AF\u03C4\u03B1\u03B9 \u03CC\u03C4\u03B9 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C0\u03C5\u03C1\u03AE\u03BD\u03B1\u03C2 \u03B5\u03BD\u03CC\u03C2 \u03B3\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1 \u03C0\u03BF\u03C5 \u03B1\u03C0\u03BF\u03C1\u03C1\u03BF\u03C6\u03AE\u03B8\u03B7\u03BA\u03B5 \u03B1\u03C0\u03CC \u03C4\u03BF\u03BD \u0393\u03B1\u03BB\u03B1\u03BE\u03AF\u03B1. \u03A0\u03B9\u03B8\u03B1\u03BD\u03CC\u03BD \u03B1\u03C5\u03C4\u03AE \u03B7 \u03C0\u03BF\u03B9\u03BA\u03B9\u03BB\u03AF\u03B1 \u03BD\u03B1 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03B1\u03C0\u03BF\u03C4\u03AD\u03BB\u03B5\u03C3\u03BC\u03B1 \u03C4\u03B7\u03C2 \u03C3\u03C5\u03B3\u03C7\u03CE\u03BD\u03B5\u03C5\u03C3\u03B7\u03C2 \u03B4\u03CD\u03BF \u03C3\u03BC\u03B7\u03BD\u03CE\u03BD \u03C3\u03B5 \u03AD\u03BD\u03B1. \u03A3\u03C4\u03BF NGC 1851 \u03B5\u03C0\u03AF\u03C3\u03B7\u03C2 \u03B2\u03C1\u03AF\u03C3\u03BA\u03B5\u03C4\u03B1\u03B9 \u03BC\u03AF\u03B1 \u03C0\u03B7\u03B3\u03AE \u03B1\u03BA\u03C4\u03B9\u03BD\u03CE\u03BD-\u03A7, \u03B7 4U 0513-40, \u03B7 \u03BF\u03C0\u03BF\u03AF\u03B1 \u03C0\u03B9\u03B8\u03B1\u03BD\u03CC\u03BD \u03BD\u03B1 \u03B5\u03AF\u03BD\u03B1\u03B9 \u03C5\u03C0\u03B5\u03C1\u03C3\u03C5\u03BC\u03C0\u03C5\u03BA\u03BD\u03C9\u03BC\u03AD\u03BD\u03BF\u03C2 \u03B4\u03B9\u03C0\u03BB\u03CC\u03C2 \u03B1\u03C3\u03C4\u03AD\u03C1\u03B1\u03C2, \u03BC\u03B5 \u03C0\u03B5\u03C1\u03AF\u03BF\u03B4\u03BF \u03C0\u03B5\u03C1\u03B9\u03C6\u03BF\u03C1\u03AC\u03C2 17 \u03BB\u03B5\u03C0\u03C4\u03AC."@el . . . . . . "NGC 1851"@zh . . . "NGC 1851 izar kumulu bat da, Columba konstelazioan. aurkitu zuen 1826ko maiatzaren\u202F10an."@eu . . "NGC 1851"@en . . "NGC 1851 (noto anche come C 73) \u00E8 un ammasso globulare visibile nella costellazione della Colomba. Visibile appena con un binocolo, un telescopio di 150mm di apertura gi\u00E0 inizia a mostrare le componenti pi\u00F9 brillanti; tuttavia il centro dell'ammasso, esteso su 5' d'arco, \u00E8 estremamente concentrato, al punto che diventa impossibile risolverlo neppure con i pi\u00F9 potenti telescopi amatoriali e semiprofessionali. NGC 1851 ha una magnitudine assoluta di -8,25, e dista dal Sole quasi 40.000 anni-luce. NGC 1851 fa parte della Salsiccia di Gaia, una galassia nana fusasi con la Via lattea circa 8, 11 miliardi di anni fa."@it . . "NGC 1851"@de . "NGC 1851 es un c\u00FAmulo globular ubicado en la constelaci\u00F3n de Columba, la Paloma. Se lo conoce tambi\u00E9n como Caldwell 73. Su magnitud aparente es de 7.3Est\u00E1 a 39,500 al,\u200B y se ubica a unos 8\u00B0 al sudoeste de la estrella de magnitud 2.65 Phact (\u03B1 Columbae)."@es . .