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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 −9 km/s, having come to within 212.5 ly some 3.12 million years ago.

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  • WW Aurigae (es)
  • WW Aurigae (en)
  • WW Возничего (ru)
  • HD46052 (uk)
  • 御夫座WW (zh)
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  • WW Возничего (лат. WW Aurigae), HD 46052 — двойная затменная переменная звезда типа Алголя (EA) в созвездии Возничего на расстоянии приблизительно 297 световых лет (около 91 парсека) от Солнца. Видимая звёздная величина звезды — от +6,54m до +5,86m. Орбитальный период — около 2,5251 суток. Возраст звезды оценивается как около 565 млн лет. (ru)
  • 御夫座WW,又名BD+32 1324,HD 46052、SAO 59194、HR 2372,是御夫座的一颗恒星,视星等为5.87,位于銀經181.72,銀緯10.52,其B1900.0坐标为赤經6h 25m 55.6s,赤緯+32° 10.52′ 34″。 (zh)
  • HD46052 — хімічно пекулярна зоря спектрального класу A2, що має видиму зоряну величину в смузі V приблизно 5,8.Вона розташована на відстані близько 275,0 світлових років від Сонця. (uk)
  • WW Aurigae (WW Aur)​ es una estrella variable de la constelación de Auriga que se encuentra a 275 años luz del Sistema Solar. WW Aurigae es una binaria eclipsante cuya naturaleza fue descubierta independientemente por Soloviev (1918) y Schwab (1918).​ Sus componentes son dos estrellas blancas de la secuencia principal de tipo espectral A3m, ambas estrellas con líneas metálicas. 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 más pequeña, tiene una masa de 1,92 masas solares, un radio de 1,84 radios solares y una temperatura de 7670 K.​La velocidad de rotación proyectada de ambas componentes es de aproximadamente 36 km/s.La componente A es 13,4 veces más luminosa que el Sol mientras que su (es)
  • 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 −9 km/s, having come to within 212.5 ly some 3.12 million years ago. (en)
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  • WW Aurigae (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/WWAurLightCurve.png
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