"225"^^ . . . . . . "NGC 2655 = Arp 225 ist eine linsenf\u00F6rmige Galaxie vom Hubble-Typ SB0/a im Sternbild Giraffe am Nordsternhimmel. Sie ist sch\u00E4tzungsweise 69 Millionen Lichtjahre von der Milchstra\u00DFe entfernt und hat einen Durchmesser von etwa 95.000 Lj.Gemeinsam mit NGC 2591, NGC 2715, NGC 2748 und drei weiteren Galaxien bildet sie die NGC-2655-Gruppe. Halton Arp gliederte seinen Katalog ungew\u00F6hnlicher Galaxien nach rein morphologischen Kriterien in Gruppen. Diese Galaxie geh\u00F6rt zu der Klasse Galaxien mit amorphen Spiralarmen. Die Typ-Ia-Supernova SN 2011B wurde hier beobachtet. Das Objekt wurde am 26. September 1802 von dem deutsch-britischen Astronomen William Herschel entdeckt."@de . . . . "NGC 2655"@en . . "63"^^ . . . "NGC 2655 (\u0434\u0440\u0443\u0433\u0438\u0435 \u043E\u0431\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u2014 UGC 4637, IRAS08491+7824, MCG 13-7-10, ZWG 350.7, ZWG 349.33, ARP 225, PGC 25069) \u2014 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0416\u0438\u0440\u0430\u0444. \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. \u0412 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0435 \u0432\u0441\u043F\u044B\u0445\u043D\u0443\u043B\u0430 \u0441\u0432\u0435\u0440\u0445\u043D\u043E\u0432\u0430\u044F SN 2011B \u0442\u0438\u043F\u0430 Ia, \u0435\u0451 \u043F\u0438\u043A\u043E\u0432\u0430\u044F \u0432\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0441\u043E\u0441\u0442\u0430\u0432\u0438\u043B\u0430 15,8. \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 NGC 2655 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0441\u043E\u0441\u0442\u0430\u0432 \u0433\u0440\u0443\u043F\u043F\u044B \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A NGC 2655. \u041F\u043E\u043C\u0438\u043C\u043E NGC 2655 \u0432 \u0433\u0440\u0443\u043F\u043F\u0443 \u0442\u0430\u043A\u0436\u0435 \u0432\u0445\u043E\u0434\u044F\u0442 NGC 2591, NGC 2715, NGC 2748, , \u0438 ."@ru . . . . "NGC 2655 is een balkspiraalstelsel in het sterrenbeeld Giraffe. Het hemelobject werd op 26 september 1802 ontdekt door de Duits-Britse astronoom William Herschel."@nl . "NGC 2655"@nl . . "NGC 2655 \u00E8 una galassia lenticolare situata nella costellazione della Giraffa alla distanza di 63 milioni di anni luce dalla Terra ed \u00E8 membro dell'omonimo . \u00C8 una galassia di Seyfert, un tipo di galassie con nucleo galattico attivo con righe spettrali caratteristiche per la presenza di gas ad alta ionizzazione. La galassia presenta nel centro strie di polvere a disposizione asimmetrica, bracci di marea, grandi quantit\u00E0 di gas di idrogeno neutro e probabilmente vi \u00E8 stato un recente evento di fusione con un'altra galassia. Anzi, dall'insieme delle caratteristiche di NGC 2655, si \u00E8 avanzata l'ipotesi che la galassia abbia avuto vari episodi di fusione con altre galassie. Allo studio nella banda dell'infrarosso \u00E8 stata evidenziata la presenza di debole barra centrale. Una scia di gas \u00E8 indir"@it . . "NGC 2655 \u2014 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0442\u0438\u043F\u0443 SB0-a \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0416\u0438\u0440\u0430\u0444. \u0412\u0456\u0434\u043A\u0440\u0438\u0432\u0430\u0447\u0435\u043C \u0446\u044C\u043E\u0433\u043E \u043E\u0431'\u0454\u043A\u0442\u0430 \u0454 \u0424\u0440\u0456\u0434\u0440\u0456\u0445 \u0412\u0456\u043B\u044C\u0433\u0435\u043B\u044C\u043C \u0413\u0435\u0440\u0448\u0435\u043B\u044C, \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 26 \u0432\u0435\u0440\u0435\u0441\u043D\u044F 1802. \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 2655 galaxia bat da, Camelopardalis konstelazioan. William Herschelek aurkitu zuen 1802ko irailaren\u202F26an."@eu . "NGC2655"@en . . "NGC 2655"@it . . . . . "NGC 2655"@sv . . . . . "NGC 2655 (r\u00F3wnie\u017C PGC 25069, UGC 4637 lub Arp 225) \u2013 galaktyka soczewkowata (SB0-a), znajduj\u0105ca si\u0119 w gwiazdozbiorze \u017Byrafy. Zosta\u0142a odkryta 26 wrze\u015Bnia 1802 roku przez Williama Herschela. Jest to galaktyka aktywna typu Seyfert 2 lub . W galaktyce tej zaobserwowano supernow\u0105 SN 2011B."@pl . "1400"^^ . . . . . . "NGC 2655 is a lenticular galaxy in the constellation Camelopardalis. It is at a distance of 60 million light years from Earth. NGC 2655 is a Seyfert galaxy. The galaxy has asymmetric dust lanes in the centre of the galaxy, tidal arms and extended neutral hydrogen gas and may have recently experienced a merger. The complex dynamics of the HI and optical tails suggest the galaxy may have undergone more mergers in the past. A weak bar has been detected in infrared H band. The diameter of the disk of the galaxy is estimated to be 60 Kpc (195,000 ly). William Herschel discovered NGC 2655 in September 26, 1802 and described it as very bright and considerably large. The galaxy can be glimpsed with a 4-inch telescope under dark skies nearly 10\u00B0 from the north celestial pole. One supernova has been observed in NGC 2655, SN 2011B, a type Ia with peak magnitude 12.8. NGC 2655 is the brightest member of the NGC 2655 group, which also contains the Sc galaxy NGC 2715, , and NGC 2748. One of the gas structures of NGC 2655 is trailing off toward the small galaxy UGC 4714."@en . . "Arp 225, UGC 4637, PGC 25069"@en . "NGC 2655 \u2014 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0442\u0438\u043F\u0443 SB0-a \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u0416\u0438\u0440\u0430\u0444. \u0412\u0456\u0434\u043A\u0440\u0438\u0432\u0430\u0447\u0435\u043C \u0446\u044C\u043E\u0433\u043E \u043E\u0431'\u0454\u043A\u0442\u0430 \u0454 \u0424\u0440\u0456\u0434\u0440\u0456\u0445 \u0412\u0456\u043B\u044C\u0433\u0435\u043B\u044C\u043C \u0413\u0435\u0440\u0448\u0435\u043B\u044C, \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 26 \u0432\u0435\u0440\u0435\u0441\u043D\u044F 1802. \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 . . . . "250"^^ . "1102403308"^^ . . . "NGC 2655"@en . "NGC 2655 is a lenticular galaxy in the constellation Camelopardalis. It is at a distance of 60 million light years from Earth. NGC 2655 is a Seyfert galaxy. The galaxy has asymmetric dust lanes in the centre of the galaxy, tidal arms and extended neutral hydrogen gas and may have recently experienced a merger. The complex dynamics of the HI and optical tails suggest the galaxy may have undergone more mergers in the past. A weak bar has been detected in infrared H band. The diameter of the disk of the galaxy is estimated to be 60 Kpc (195,000 ly)."@en . "4637"^^ . . . . . . . . "NGC 2655"@ru . . . . . . . "NGC 2655 galaxia bat da, Camelopardalis konstelazioan. William Herschelek aurkitu zuen 1802ko irailaren\u202F26an."@eu . . . "NGC 2655 \u0647\u064A \u0645\u062C\u0631\u0629 \u0645\u062D\u062F\u0628\u0629 \u062A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0632\u0631\u0627\u0641\u0629. \u062A\u0628\u0639\u062F \u062D\u0648\u0627\u0644\u064A \u0645\u0633\u0627\u0641\u0629 60 \u0645\u0644\u064A\u0648\u0646 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u0645\u0646 \u0627\u0644\u0623\u0631\u0636. NGC 2655 \u0645\u062C\u0631\u0629 \u0632\u0627\u064A\u0641\u0631\u062A \u0648\u0627\u0644\u0645\u062C\u0631\u0629 \u0644\u062F\u064A\u0647\u0627 \u0645\u0645\u0631\u0627\u062A \u0627\u0644\u063A\u0628\u0627\u0631 \u063A\u064A\u0631 \u0627\u0644\u0645\u062A\u0645\u0627\u062B\u0644\u0629 \u0641\u064A \u0648\u0633\u0637 \u0627\u0644\u0645\u062C\u0631\u0629 \u0648\u0627\u0644\u0645\u062F \u0648\u0627\u0644\u062C\u0632\u0631 \u0648\u063A\u0627\u0632 \u0627\u0644\u0647\u064A\u062F\u0631\u0648\u062C\u064A\u0646 \u0648\u0631\u0628\u0645\u0627 \u0634\u0647\u062F\u062A \u0645\u0624\u062E\u0631\u0627 \u0627\u0644\u0627\u0646\u062F\u0645\u0627\u062C. \u0627\u0644\u0645\u062C\u0631\u0629 \u0642\u062F \u062A\u0643\u0648\u0646 \u0642\u062F \u062E\u0636\u0639\u062A \u0644\u0645\u0632\u064A\u062F \u0645\u0646 \u0639\u0645\u0644\u064A\u0627\u062A \u0627\u0644\u0627\u0646\u062F\u0645\u0627\u062C \u0641\u064A \u0627\u0644\u0645\u0627\u0636\u064A. \u062A\u0645 \u0627\u0644\u0643\u0634\u0641 \u0639\u0646 \u0634\u0631\u064A\u0637 \u0636\u0639\u064A\u0641 \u0641\u064A \u0627\u0644\u0623\u0634\u0639\u0629 \u062A\u062D\u062A \u0627\u0644\u062D\u0645\u0631\u0627\u0621 \u0648\u064A\u0642\u062F\u0631 \u0642\u0637\u0631 \u0642\u0631\u0635 \u0627\u0644\u0645\u062C\u0631\u0629 \u0628 60 \u0643\u064A\u0644\u0648\u0628\u0627\u064A\u062A 195,000 ly. \u0627\u0643\u062A\u0634\u0641\u0647\u0627 \u0639\u0627\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0648\u064A\u0644\u064A\u0627\u0645 \u0647\u064A\u0631\u0634\u064A\u0644 \u0641\u064A 26 \u0633\u0628\u062A\u0645\u0628\u0631 1802 \u0648\u0648\u0635\u0641\u0647\u0627 \u0628\u0623\u0646\u0647\u0627 \u0645\u0634\u0631\u0642\u0629 \u062C\u062F\u0627 \u0648\u0643\u0628\u064A\u0631\u0629 \u0625\u0644\u0649 \u062D\u062F \u0643\u0628\u064A\u0631. \u0644\u0648\u062D\u0638 \u0623\u062D\u062F \u0627\u0644\u0645\u0633\u062A\u0639\u0631\u0627\u062A \u0627\u0644\u0623\u0639\u0638\u0645 \u0641\u064A 2011 \u0648\u0647\u0648 \u0645\u0646 \u0646\u0648\u0639 \u0645\u0633\u062A\u0639\u0631 \u0623\u0639\u0638\u0645 \u0646\u0648\u0639 1\u0623 \u0645\u0639 \u062D\u062C\u0645 12,8. NGC 2655 \u0647\u0648 \u0623\u0644\u0645\u0639 \u0639\u0636\u0648 \u0641\u064A \u0645\u062C\u0645\u0648\u0639\u0629 NGC 2655 \u0648\u0627\u0644\u062A\u064A \u062A\u062D\u062A\u0648\u064A \u0623\u064A\u0636\u0627 \u0639\u0644\u0649 \u0627\u0644\u0645\u062C\u0631\u0629 NGC 2715 , NGC 2591, \u0648 NGC 2748. \u0648\u0627\u062D\u062F\u0629 \u0645\u0646 \u0647\u064A\u0627\u0643\u0644 \u0627\u0644\u063A\u0627\u0632 \u064A\u062A\u062C\u0647 \u0646\u062D\u0648 \u0627\u0644\u0645\u062C\u0631\u0629 \u0627\u0644\u0635\u063A\u064A\u0631\u0629 UGC 4714."@ar . "NGC 2655 (r\u00F3wnie\u017C PGC 25069, UGC 4637 lub Arp 225) \u2013 galaktyka soczewkowata (SB0-a), znajduj\u0105ca si\u0119 w gwiazdozbiorze \u017Byrafy. Zosta\u0142a odkryta 26 wrze\u015Bnia 1802 roku przez Williama Herschela. Jest to galaktyka aktywna typu Seyfert 2 lub . W galaktyce tej zaobserwowano supernow\u0105 SN 2011B."@pl . . "NGC 2655 \u00E9 uma gal\u00E1xia espiral localizada a cerca de setenta e um milh\u00F5es de anos-luz (aproximadamente 21,76 megaparsecs) de dist\u00E2ncia na dire\u00E7\u00E3o da constela\u00E7\u00E3o da Girafa. Possui uma magnitude aparente de 10,1, uma declina\u00E7\u00E3o de +78\u00BA 13' 24\" e uma ascens\u00E3o reta de 08 horas, 55 minutos e 38,4 segundos."@pt . "NGC 2655"@eo . "NGC 2655"@ar . "NGC 2655 \u0647\u064A \u0645\u062C\u0631\u0629 \u0645\u062D\u062F\u0628\u0629 \u062A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0632\u0631\u0627\u0641\u0629. \u062A\u0628\u0639\u062F \u062D\u0648\u0627\u0644\u064A \u0645\u0633\u0627\u0641\u0629 60 \u0645\u0644\u064A\u0648\u0646 \u0633\u0646\u0629 \u0636\u0648\u0626\u064A\u0629 \u0645\u0646 \u0627\u0644\u0623\u0631\u0636. NGC 2655 \u0645\u062C\u0631\u0629 \u0632\u0627\u064A\u0641\u0631\u062A \u0648\u0627\u0644\u0645\u062C\u0631\u0629 \u0644\u062F\u064A\u0647\u0627 \u0645\u0645\u0631\u0627\u062A \u0627\u0644\u063A\u0628\u0627\u0631 \u063A\u064A\u0631 \u0627\u0644\u0645\u062A\u0645\u0627\u062B\u0644\u0629 \u0641\u064A \u0648\u0633\u0637 \u0627\u0644\u0645\u062C\u0631\u0629 \u0648\u0627\u0644\u0645\u062F \u0648\u0627\u0644\u062C\u0632\u0631 \u0648\u063A\u0627\u0632 \u0627\u0644\u0647\u064A\u062F\u0631\u0648\u062C\u064A\u0646 \u0648\u0631\u0628\u0645\u0627 \u0634\u0647\u062F\u062A \u0645\u0624\u062E\u0631\u0627 \u0627\u0644\u0627\u0646\u062F\u0645\u0627\u062C. \u0627\u0644\u0645\u062C\u0631\u0629 \u0642\u062F \u062A\u0643\u0648\u0646 \u0642\u062F \u062E\u0636\u0639\u062A \u0644\u0645\u0632\u064A\u062F \u0645\u0646 \u0639\u0645\u0644\u064A\u0627\u062A \u0627\u0644\u0627\u0646\u062F\u0645\u0627\u062C \u0641\u064A \u0627\u0644\u0645\u0627\u0636\u064A. \u062A\u0645 \u0627\u0644\u0643\u0634\u0641 \u0639\u0646 \u0634\u0631\u064A\u0637 \u0636\u0639\u064A\u0641 \u0641\u064A \u0627\u0644\u0623\u0634\u0639\u0629 \u062A\u062D\u062A \u0627\u0644\u062D\u0645\u0631\u0627\u0621 \u0648\u064A\u0642\u062F\u0631 \u0642\u0637\u0631 \u0642\u0631\u0635 \u0627\u0644\u0645\u062C\u0631\u0629 \u0628 60 \u0643\u064A\u0644\u0648\u0628\u0627\u064A\u062A 195,000 ly. \u0627\u0643\u062A\u0634\u0641\u0647\u0627 \u0639\u0627\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0648\u064A\u0644\u064A\u0627\u0645 \u0647\u064A\u0631\u0634\u064A\u0644 \u0641\u064A 26 \u0633\u0628\u062A\u0645\u0628\u0631 1802 \u0648\u0648\u0635\u0641\u0647\u0627 \u0628\u0623\u0646\u0647\u0627 \u0645\u0634\u0631\u0642\u0629 \u062C\u062F\u0627 \u0648\u0643\u0628\u064A\u0631\u0629 \u0625\u0644\u0649 \u062D\u062F \u0643\u0628\u064A\u0631. \u0644\u0648\u062D\u0638 \u0623\u062D\u062F \u0627\u0644\u0645\u0633\u062A\u0639\u0631\u0627\u062A \u0627\u0644\u0623\u0639\u0638\u0645 \u0641\u064A 2011 \u0648\u0647\u0648 \u0645\u0646 \u0646\u0648\u0639 \u0645\u0633\u062A\u0639\u0631 \u0623\u0639\u0638\u0645 \u0646\u0648\u0639 1\u0623 \u0645\u0639 \u062D\u062C\u0645 12,8."@ar . "NGC 2655 (aliaj indikoj \u2014 UGC 4637, IRAS08491+7824, MCG 13-7-10, ZWG 350.7, ZWG 349.33, ARP 225, PGC 25069) estas galaksio en konstelacio \u011Cirafo. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo."@eo . . . . . "NGC 2655"@uk . . . . "25069"^^ . "NGC 2655 \u00E4r en stavgalax i stj\u00E4rnbilden Giraffen. Den uppt\u00E4cktes den 26 september 1802 av William Herschel."@sv . . . "49210115"^^ . . "4"^^ . . . . "NGC 2655 (\u0434\u0440\u0443\u0433\u0438\u0435 \u043E\u0431\u043E\u0437\u043D\u0430\u0447\u0435\u043D\u0438\u044F \u2014 UGC 4637, IRAS08491+7824, MCG 13-7-10, ZWG 350.7, ZWG 349.33, ARP 225, PGC 25069) \u2014 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0416\u0438\u0440\u0430\u0444. \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. \u0412 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0435 \u0432\u0441\u043F\u044B\u0445\u043D\u0443\u043B\u0430 \u0441\u0432\u0435\u0440\u0445\u043D\u043E\u0432\u0430\u044F SN 2011B \u0442\u0438\u043F\u0430 Ia, \u0435\u0451 \u043F\u0438\u043A\u043E\u0432\u0430\u044F \u0432\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0441\u043E\u0441\u0442\u0430\u0432\u0438\u043B\u0430 15,8. \u0413\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u0430 NGC 2655 \u0432\u0445\u043E\u0434\u0438\u0442 \u0432 \u0441\u043E\u0441\u0442\u0430\u0432 \u0433\u0440\u0443\u043F\u043F\u044B \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A NGC 2655. \u041F\u043E\u043C\u0438\u043C\u043E NGC 2655 \u0432 \u0433\u0440\u0443\u043F\u043F\u0443 \u0442\u0430\u043A\u0436\u0435 \u0432\u0445\u043E\u0434\u044F\u0442 NGC 2591, NGC 2715, NGC 2748, , \u0438 . \u042F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u043E\u0439 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u043E\u0439 \u0441 \u043F\u0440\u0438\u0437\u043D\u0430\u043A\u0430\u043C\u0438 \u043D\u0435\u0434\u0430\u0432\u043D\u0435\u0433\u043E \u043A\u0440\u0443\u043F\u043D\u043E\u0433\u043E \u0441\u043B\u0438\u044F\u043D\u0438\u044F \u0441 \u0434\u0440\u0443\u0433\u043E\u0439 \u0433\u0430\u043B\u0430\u043A\u0442\u0438\u043A\u043E\u0439. \u0412 \u043D\u0435\u0439 \u0432\u0441\u0451 \u0435\u0449\u0451 \u043C\u043E\u0433\u0443\u0442 \u043F\u0440\u043E\u0434\u043E\u043B\u0436\u0430\u0442\u044C\u0441\u044F \u0437\u0432\u0451\u0437\u0434\u043E\u043E\u0431\u0440\u0430\u0437\u043E\u0432\u0430\u043D\u0438\u0435 \u0438 \u0444\u043E\u0440\u043C\u0438\u0440\u043E\u0432\u0430\u043D\u0438\u0435 \u043D\u043E\u0432\u044B\u0445 \u0437\u0432\u0451\u0437\u0434\u043D\u044B\u0445 \u0441\u043A\u043E\u043F\u043B\u0435\u043D\u0438\u0439. NGC 2655 \u043C\u043E\u0436\u0435\u0442 \u0431\u044B\u0442\u044C \u043F\u0440\u0438\u043C\u0435\u0440\u043E\u043C \u0442\u043E\u0433\u043E, \u043A\u0430\u043A \u0431\u0443\u0434\u0435\u0442 \u0432\u044B\u0433\u043B\u044F\u0434\u0435\u0442\u044C \u041C\u043B\u0435\u0447\u043D\u044B\u0439 \u041F\u0443\u0442\u044C \u043F\u043E\u0441\u043B\u0435 \u0441\u0442\u043E\u043B\u043A\u043D\u043E\u0432\u0435\u043D\u0438\u044F \u0438 \u0441\u043B\u0438\u044F\u043D\u0438\u044F \u0441 \u0422\u0443\u043C\u0430\u043D\u043D\u043E\u0441\u0442\u044C\u044E \u0410\u043D\u0434\u0440\u043E\u043C\u0435\u0434\u044B."@ru . "NGC 2655"@de . . . . . . . . "Arp225,UGC4637,PGC25069"@en . . . "NGC 2655 \u00E9 uma gal\u00E1xia espiral localizada a cerca de setenta e um milh\u00F5es de anos-luz (aproximadamente 21,76 megaparsecs) de dist\u00E2ncia na dire\u00E7\u00E3o da constela\u00E7\u00E3o da Girafa. Possui uma magnitude aparente de 10,1, uma declina\u00E7\u00E3o de +78\u00BA 13' 24\" e uma ascens\u00E3o reta de 08 horas, 55 minutos e 38,4 segundos."@pt . . "NGC 2655 is een balkspiraalstelsel in het sterrenbeeld Giraffe. Het hemelobject werd op 26 september 1802 ontdekt door de Duits-Britse astronoom William Herschel."@nl . "NGC 2655"@pl . . . . "10.1"^^ . . . "NGC 2655"@fr . "NGC 2655 = Arp 225 ist eine linsenf\u00F6rmige Galaxie vom Hubble-Typ SB0/a im Sternbild Giraffe am Nordsternhimmel. Sie ist sch\u00E4tzungsweise 69 Millionen Lichtjahre von der Milchstra\u00DFe entfernt und hat einen Durchmesser von etwa 95.000 Lj.Gemeinsam mit NGC 2591, NGC 2715, NGC 2748 und drei weiteren Galaxien bildet sie die NGC-2655-Gruppe. Halton Arp gliederte seinen Katalog ungew\u00F6hnlicher Galaxien nach rein morphologischen Kriterien in Gruppen. Diese Galaxie geh\u00F6rt zu der Klasse Galaxien mit amorphen Spiralarmen. Die Typ-Ia-Supernova SN 2011B wurde hier beobachtet."@de . . "NGC 2655 by Hubble Space Telescope."@en . . . "NGC 2655 est une vaste galaxie lenticulaire situ\u00E9e dans la constellation de la Girafe. Sa vitesse par rapport au fond diffus cosmologique est de (1 418 \u00B1 2) km/s, ce qui correspond \u00E0 une distance de Hubble de 20,9 \u00B1 1,5 Mpc (\u223C68,2 millions d'a.l.). NGC 2655 a \u00E9t\u00E9 d\u00E9couverte par l'astronome germano-britannique William Herschel en 1802. NGC 2655 est une galaxie LINER, c'est-\u00E0-dire une galaxie dont le noyau pr\u00E9sente un spectre d'\u00E9mission caract\u00E9ris\u00E9 par de larges raies d'atomes faiblement ionis\u00E9s et elle pr\u00E9sente une large raie HI. C'est une galaxie active de type Seyfert 2."@fr . . "2655"^^ . . . . "NGC 2655 \u00E4r en stavgalax i stj\u00E4rnbilden Giraffen. Den uppt\u00E4cktes den 26 september 1802 av William Herschel."@sv . . . . "NGC 2655"@eu . . "4237"^^ . . . . . "NGC 2655 (aliaj indikoj \u2014 UGC 4637, IRAS08491+7824, MCG 13-7-10, ZWG 350.7, ZWG 349.33, ARP 225, PGC 25069) estas galaksio en konstelacio \u011Cirafo. \u0108i tiu objekto estis jam en la originala versio de NGC-katalogo."@eo . "NGC 2655 \u00E8 una galassia lenticolare situata nella costellazione della Giraffa alla distanza di 63 milioni di anni luce dalla Terra ed \u00E8 membro dell'omonimo . \u00C8 una galassia di Seyfert, un tipo di galassie con nucleo galattico attivo con righe spettrali caratteristiche per la presenza di gas ad alta ionizzazione. La galassia presenta nel centro strie di polvere a disposizione asimmetrica, bracci di marea, grandi quantit\u00E0 di gas di idrogeno neutro e probabilmente vi \u00E8 stato un recente evento di fusione con un'altra galassia. Anzi, dall'insieme delle caratteristiche di NGC 2655, si \u00E8 avanzata l'ipotesi che la galassia abbia avuto vari episodi di fusione con altre galassie. Allo studio nella banda dell'infrarosso \u00E8 stata evidenziata la presenza di debole barra centrale. Una scia di gas \u00E8 indirizzata versa la vicina piccola galassia . Il diametro di NGC 2655 \u00E8 maggiore di quello della Via Lattea, raggiungendo circa 195.000 anni luce. NGC 2655 \u00E8 il membro pi\u00F9 luminoso del gruppo di NGC 2655 che contiene, tra le altre, le galassie , e . Nel 2011 \u00E8 stata osservata la supernova , una supernova di tipo Ia con picco di magnitudine di 12,8."@it . "SAB0/a"@en . "NGC 2655"@pt . . "NGC 2655 est une vaste galaxie lenticulaire situ\u00E9e dans la constellation de la Girafe. Sa vitesse par rapport au fond diffus cosmologique est de (1 418 \u00B1 2) km/s, ce qui correspond \u00E0 une distance de Hubble de 20,9 \u00B1 1,5 Mpc (\u223C68,2 millions d'a.l.). NGC 2655 a \u00E9t\u00E9 d\u00E9couverte par l'astronome germano-britannique William Herschel en 1802. NGC 2655 est une galaxie LINER, c'est-\u00E0-dire une galaxie dont le noyau pr\u00E9sente un spectre d'\u00E9mission caract\u00E9ris\u00E9 par de larges raies d'atomes faiblement ionis\u00E9s et elle pr\u00E9sente une large raie HI. C'est une galaxie active de type Seyfert 2. \u00C0 ce jour, une mesure non bas\u00E9e sur le d\u00E9calage vers le rouge (redshift) donne une distance d'environ 24,400 Mpc (\u223C79,6 millions d'a.l.). Cette valeur est \u00E0 l'ext\u00E9rieur mais compatible avec les valeurs de la distance de Hubble."@fr .