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- EO Aurigae is an eclipsing binary of Algol type in the northern constellation of Auriga. With a combined apparent magnitude of 7.71, it is too faint to be seen with the unaided eye. The eclipsing binary nature of the star was detected in 1943 by Sergei Gaposchkin at Harvard College Observatory. It consists of a pair of B-type main sequence stars orbiting each other with a period of 4.0656 days. During the eclipse of the primary star, the combined magnitude drops by 0.57; the eclipse of the secondary component drops the magnitude by 0.33. (en)
- EO Возничего (лат. EO Aurigae), HD 34333 — двойная затменная переменная звезда типа Алголя (EA) в созвездии Возничего на расстоянии приблизительно 4152 световых лет (около 1273 парсеков) от Солнца. Видимая звёздная величина звезды — от +8,13m до +7,56m. Орбитальный период — около 4,0656 суток. Возраст звезды оценивается как около 23,6 млн лет. (ru)
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- EO Aur A (en)
- EO Aur B (en)
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- EO Aurigae is an eclipsing binary of Algol type in the northern constellation of Auriga. With a combined apparent magnitude of 7.71, it is too faint to be seen with the unaided eye. The eclipsing binary nature of the star was detected in 1943 by Sergei Gaposchkin at Harvard College Observatory. It consists of a pair of B-type main sequence stars orbiting each other with a period of 4.0656 days. During the eclipse of the primary star, the combined magnitude drops by 0.57; the eclipse of the secondary component drops the magnitude by 0.33. (en)
- EO Возничего (лат. EO Aurigae), HD 34333 — двойная затменная переменная звезда типа Алголя (EA) в созвездии Возничего на расстоянии приблизительно 4152 световых лет (около 1273 парсеков) от Солнца. Видимая звёздная величина звезды — от +8,13m до +7,56m. Орбитальный период — около 4,0656 суток. Возраст звезды оценивается как около 23,6 млн лет. (ru)
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- EO Aurigae (en)
- EO Возничего (ru)
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