IU Aurigae is a triple star system in the constellation Auriga, consisting of an eclipsing binary pair orbiting a third component with a period of 335 years. This system is too faint to be viewed with the naked eye, having a peak apparent visual magnitude of 8.19. The eclipsing pair form a Beta Lyrae-type semidetached binary of two Bp stars with a period of 1.81147435 days. During the primary eclipse, the visual magnitude of the system drops to 8.89, while for the secondary it decreases to 8.74. The third component is a massive object with 17–18 M☉, and may actually be a binary – which would make this a quadruple star system.
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| - IU Aurigae (en)
- IU Возничего (ru)
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| - IU Aurigae is a triple star system in the constellation Auriga, consisting of an eclipsing binary pair orbiting a third component with a period of 335 years. This system is too faint to be viewed with the naked eye, having a peak apparent visual magnitude of 8.19. The eclipsing pair form a Beta Lyrae-type semidetached binary of two Bp stars with a period of 1.81147435 days. During the primary eclipse, the visual magnitude of the system drops to 8.89, while for the secondary it decreases to 8.74. The third component is a massive object with 17–18 M☉, and may actually be a binary – which would make this a quadruple star system. (en)
- IU Возничего (лат. IU Aurigae), HD 35652 — тройная звезда в созвездии Возничего на расстоянии (вычисленном из значения параллакса) приблизительно 6815 световых лет (около 2089 парсеков) от Солнца. Видимая звёздная величина звезды — от +8,89m до +8,19m. Пара первого и второго компонентов — двойная затменная переменная звезда типа Беты Лиры (EB). Орбитальный период — около 1,8115 суток. (ru)
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| - IU Aurigae is a triple star system in the constellation Auriga, consisting of an eclipsing binary pair orbiting a third component with a period of 335 years. This system is too faint to be viewed with the naked eye, having a peak apparent visual magnitude of 8.19. The eclipsing pair form a Beta Lyrae-type semidetached binary of two Bp stars with a period of 1.81147435 days. During the primary eclipse, the visual magnitude of the system drops to 8.89, while for the secondary it decreases to 8.74. The third component is a massive object with 17–18 M☉, and may actually be a binary – which would make this a quadruple star system. (en)
- IU Возничего (лат. IU Aurigae), HD 35652 — тройная звезда в созвездии Возничего на расстоянии (вычисленном из значения параллакса) приблизительно 6815 световых лет (около 2089 парсеков) от Солнца. Видимая звёздная величина звезды — от +8,89m до +8,19m. Пара первого и второго компонентов — двойная затменная переменная звезда типа Беты Лиры (EB). Орбитальный период — около 1,8115 суток. (ru)
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