. . . "WW \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. WW Aurigae), HD 46052 \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0430\u0442\u043C\u0435\u043D\u043D\u0430\u044F \u043F\u0435\u0440\u0435\u043C\u0435\u043D\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0442\u0438\u043F\u0430 \u0410\u043B\u0433\u043E\u043B\u044F (EA) \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 297 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 91 \u043F\u0430\u0440\u0441\u0435\u043A\u0430) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 \u043E\u0442 +6,54m \u0434\u043E +5,86m. \u041E\u0440\u0431\u0438\u0442\u0430\u043B\u044C\u043D\u044B\u0439 \u043F\u0435\u0440\u0438\u043E\u0434 \u2014 \u043E\u043A\u043E\u043B\u043E 2,5251 \u0441\u0443\u0442\u043E\u043A. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u0446\u0435\u043D\u0438\u0432\u0430\u0435\u0442\u0441\u044F \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 565 \u043C\u043B\u043D \u043B\u0435\u0442."@ru . "WW Aur b"@en . . . ""@en . . "HD46052 \u2014 \u0445\u0456\u043C\u0456\u0447\u043D\u043E \u043F\u0435\u043A\u0443\u043B\u044F\u0440\u043D\u0430 \u0437\u043E\u0440\u044F \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043B\u0430\u0441\u0443 A2, \u0449\u043E \u043C\u0430\u0454 \u0432\u0438\u0434\u0438\u043C\u0443 \u0437\u043E\u0440\u044F\u043D\u0443 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0443 \u0432 \u0441\u043C\u0443\u0437\u0456 V \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u043E 5,8.\u0412\u043E\u043D\u0430 \u0440\u043E\u0437\u0442\u0430\u0448\u043E\u0432\u0430\u043D\u0430 \u043D\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u0456 \u0431\u043B\u0438\u0437\u044C\u043A\u043E 275,0 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F."@uk . "2903184"^^ . . . "218160.0"^^ . . "300.0"^^ . . . . "WW Aurigae"@en . . . . . . . . "0"^^ . . "WW Aurigae"@es . . "10.5"^^ . . "HD46052"@uk . "13.5"^^ . . . "WW \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E (\u043B\u0430\u0442. WW Aurigae), HD 46052 \u2014 \u0434\u0432\u043E\u0439\u043D\u0430\u044F \u0437\u0430\u0442\u043C\u0435\u043D\u043D\u0430\u044F \u043F\u0435\u0440\u0435\u043C\u0435\u043D\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0442\u0438\u043F\u0430 \u0410\u043B\u0433\u043E\u043B\u044F (EA) \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E 297 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 (\u043E\u043A\u043E\u043B\u043E 91 \u043F\u0430\u0440\u0441\u0435\u043A\u0430) \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0412\u0438\u0434\u0438\u043C\u0430\u044F \u0437\u0432\u0451\u0437\u0434\u043D\u0430\u044F \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 \u043E\u0442 +6,54m \u0434\u043E +5,86m. \u041E\u0440\u0431\u0438\u0442\u0430\u043B\u044C\u043D\u044B\u0439 \u043F\u0435\u0440\u0438\u043E\u0434 \u2014 \u043E\u043A\u043E\u043B\u043E 2,5251 \u0441\u0443\u0442\u043E\u043A. \u0412\u043E\u0437\u0440\u0430\u0441\u0442 \u0437\u0432\u0435\u0437\u0434\u044B \u043E\u0446\u0435\u043D\u0438\u0432\u0430\u0435\u0442\u0441\u044F \u043A\u0430\u043A \u043E\u043A\u043E\u043B\u043E 565 \u043C\u043B\u043D \u043B\u0435\u0442."@ru . . . "WW \u0412\u043E\u0437\u043D\u0438\u0447\u0435\u0433\u043E"@ru . . . . . . . . . "0"^^ . . "1.29"^^ . . . . "\u5FA1\u592B\u5EA7WW"@zh . "WW Aurigae (WW Aur)\u200B es una estrella variable de la constelaci\u00F3n de Auriga que se encuentra a 275 a\u00F1os luz del Sistema Solar. WW Aurigae es una binaria eclipsante cuya naturaleza fue descubierta independientemente por Soloviev (1918) y Schwab (1918).\u200B Sus componentes son dos estrellas blancas de la secuencia principal de tipo espectral A3m, ambas estrellas con l\u00EDneas met\u00E1licas. WW Aurigae A tiene una masa de 1,96 masas solares, un radio de 1,81 radios solares y una temperatura superficial de 7960 K. WW Aurigae B, ligeramente m\u00E1s peque\u00F1a, tiene una masa de 1,92 masas solares, un radio de 1,84 radios solares y una temperatura de 7670 K.\u200BLa velocidad de rotaci\u00F3n proyectada de ambas componentes es de aproximadamente 36 km/s.La componente A es 13,4 veces m\u00E1s luminosa que el Sol mientras que su acompa\u00F1ante es 10,5 veces m\u00E1s luminosa.\u200BLas caracter\u00EDsticas f\u00EDsicas del sistema se ajustan a modelos te\u00F3ricos de evoluci\u00F3n estelar considerando una edad de 90 millones de a\u00F1os as\u00ED como una elevada metalicidad.\u200B Regularmente una de las componentes eclipsa a la otra y el brillo conjunto disminuye de magnitud aparente +5,86 a +6,54 cada 2,525 d\u00EDas.\u200B"@es . "HD46052 \u2014 \u0445\u0456\u043C\u0456\u0447\u043D\u043E \u043F\u0435\u043A\u0443\u043B\u044F\u0440\u043D\u0430 \u0437\u043E\u0440\u044F \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043B\u0430\u0441\u0443 A2, \u0449\u043E \u043C\u0430\u0454 \u0432\u0438\u0434\u0438\u043C\u0443 \u0437\u043E\u0440\u044F\u043D\u0443 \u0432\u0435\u043B\u0438\u0447\u0438\u043D\u0443 \u0432 \u0441\u043C\u0443\u0437\u0456 V \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u043E 5,8.\u0412\u043E\u043D\u0430 \u0440\u043E\u0437\u0442\u0430\u0448\u043E\u0432\u0430\u043D\u0430 \u043D\u0430 \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u0456 \u0431\u043B\u0438\u0437\u044C\u043A\u043E 275,0 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0421\u043E\u043D\u0446\u044F."@uk . . . "\u221226.347"@en . "\u5FA1\u592B\u5EA7WW\uFF0C\u53C8\u540DBD+32 1324\uFF0CHD 46052\u3001SAO 59194\u3001HR 2372\uFF0C\u662F\u5FA1\u592B\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A5.87\uFF0C\u4F4D\u4E8E\u9280\u7D93181.72\uFF0C\u9280\u7DEF10.52\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D936h 25m 55.6s\uFF0C\u8D64\u7DEF+32\u00B0 10.52\u2032 34\u2033\u3002"@zh . . . . . "0.0829"^^ . . . . "WW Aurigae (WW Aur)\u200B es una estrella variable de la constelaci\u00F3n de Auriga que se encuentra a 275 a\u00F1os luz del Sistema Solar. WW Aurigae es una binaria eclipsante cuya naturaleza fue descubierta independientemente por Soloviev (1918) y Schwab (1918).\u200B Sus componentes son dos estrellas blancas de la secuencia principal de tipo espectral A3m, ambas estrellas con l\u00EDneas met\u00E1licas. WW Aurigae A tiene una masa de 1,96 masas solares, un radio de 1,81 radios solares y una temperatura superficial de 7960 K. WW Aurigae B, ligeramente m\u00E1s peque\u00F1a, tiene una masa de 1,92 masas solares, un radio de 1,84 radios solares y una temperatura de 7670 K.\u200BLa velocidad de rotaci\u00F3n proyectada de ambas componentes es de aproximadamente 36 km/s.La componente A es 13,4 veces m\u00E1s luminosa que el Sol mientras que su "@es . . . . "8128"^^ . "115.6"^^ . . . . . . . "WW Aurigae is an eclipsing binary star system in the northern constellation of Auriga. It has a combined maximum apparent visual magnitude of 5.86, which is bright enough to be dimly visible to the naked eye. Based upon an annual parallax shift of 11.0 mas, it is located 297 light years from the Earth. The system is moving further away with a heliocentric radial velocity of \u22129 km/s, having come to within 212.5 ly some 3.12 million years ago."@en . . . . "1079514097"^^ . "127.7"^^ . . . . . "WW Aurigae"@en . . . . . . . . . . . . . . . . . "WW Aurigae is an eclipsing binary star system in the northern constellation of Auriga. It has a combined maximum apparent visual magnitude of 5.86, which is bright enough to be dimly visible to the naked eye. Based upon an annual parallax shift of 11.0 mas, it is located 297 light years from the Earth. The system is moving further away with a heliocentric radial velocity of \u22129 km/s, having come to within 212.5 ly some 3.12 million years ago. This is a double-lined spectroscopic binary system, having a circular orbit with a period of 2.5 days. It was discovered to be variable independently by Friedrich Schwab and Heinrich Van Solowiew in 1913. Both components are metallic-lined, or Am stars, with a spectrum showing a deficiency of calcium and scandium, and an overabundance of heavier elements. Together they form an EA, or Algol-type, eclipsing binary with the primary occultation reducing the net magnitude to a minimum of 6.54 and the secondary eclipse lowering it to 6.43, over a cycle time of 2.52501936 days."@en . . . . . . . . . . . . . . . "\u5FA1\u592B\u5EA7WW\uFF0C\u53C8\u540DBD+32 1324\uFF0CHD 46052\u3001SAO 59194\u3001HR 2372\uFF0C\u662F\u5FA1\u592B\u5EA7\u7684\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A5.87\uFF0C\u4F4D\u4E8E\u9280\u7D93181.72\uFF0C\u9280\u7DEF10.52\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D936h 25m 55.6s\uFF0C\u8D64\u7DEF+32\u00B0 10.52\u2032 34\u2033\u3002"@zh . . . . . "5.82"^^ . . "\u221217.343"@en . . . "WW Aur A"@en . "J2000"@en . . . . . "10.9979"^^ .