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About: BX Andromedae

An Entity of Type: star, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org

BX Andromedae (BX And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 8.87. Within a cycle of approximately 14.6 hours, the brightness drops down to a magnitude of 9.53 during the main eclipse, and to a magnitude of 9.12 during the secondary one. It is classified as a Beta Lyrae variable.

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dbo:abstract
  • BX Andromedae (BX And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 8.87. Within a cycle of approximately 14.6 hours, the brightness drops down to a magnitude of 9.53 during the main eclipse, and to a magnitude of 9.12 during the secondary one. It is classified as a Beta Lyrae variable. (en)
  • BX Андромеды (лат. BX Andromedae), HD 13078 — тройная звезда в созвездии Андромеды на расстоянии приблизительно 597 световых лет (около 183 парсеков) от Солнца. Пара первого и второго компонентов — двойная затменная переменная звезда типа Беты Лиры (EB). Видимая звёздная величина звезды — от +9,53m до +8,87m. Орбитальный период — около 0,6101 суток (14,643 часов). (ru)
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  • J (en)
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  • K (en)
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  • Secondary (en)
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  • BX Andromedae (BX And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 8.87. Within a cycle of approximately 14.6 hours, the brightness drops down to a magnitude of 9.53 during the main eclipse, and to a magnitude of 9.12 during the secondary one. It is classified as a Beta Lyrae variable. (en)
  • BX Андромеды (лат. BX Andromedae), HD 13078 — тройная звезда в созвездии Андромеды на расстоянии приблизительно 597 световых лет (около 183 парсеков) от Солнца. Пара первого и второго компонентов — двойная затменная переменная звезда типа Беты Лиры (EB). Видимая звёздная величина звезды — от +9,53m до +8,87m. Орбитальный период — около 0,6101 суток (14,643 часов). (ru)
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  • BX Andromedae (en)
  • BX Андромеды (ru)
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