Results for aurigae translation from English to Russian

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beta aurigae

Russian

Бета Возничего

Last Update: 2014-10-29
Usage Frequency: 6
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Reference: Wikipedia

English

iota aurigae (ι aur, ι aurigae) is a star in the northern constellation of auriga.

Russian

Йота Возничего ("ι aur, ι aurigae") — оранжевый яркий гигант в созвездии Возничего.

Last Update: 2016-03-03
Usage Frequency: 1
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Reference: Wikipedia
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English

hans ludendorff, who had also been observing epsilon aurigae, was the first to conduct a detailed study of the star.

Russian

Ганс Людендорфф, который также наблюдал Эпсилон Возничего, был первым, кто провёл детальное исследование звезды.

Last Update: 2016-03-03
Usage Frequency: 1
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Reference: Wikipedia

English

epsilon aurigae has been targeted for observation by international year of astronomy observers from 2009 to 2011, the three years that overlap its next eclipse.

Russian

Наблюдения Эпсилона Возничего приурочены к Международному году астрономии и проводятся с 2009 по 2011 гг., то есть три года, на которые приходится затмение.

Last Update: 2016-03-03
Usage Frequency: 1
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Reference: Wikipedia

English

epsilon aurigae (ε aur, ε aurigae) is the bayer designation for a star in the northern constellation of auriga.

Russian

Эпсилон Возничего (ε aur / ε aurigae) — звезда в созвездии Возничего.

Last Update: 2016-03-03
Usage Frequency: 1
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Reference: Wikipedia

English

beta aurigae (β aur, β aurigae) is the bayer designation for a binary star system in the northern constellation of auriga.

Russian

Бета Возничего (β aur/β aurigae) — тройная звёздная система в созвездии Возничего.

Last Update: 2016-03-03
Usage Frequency: 1
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Reference: Wikipedia

English

in 1904, he published in "astronomische nachrichten" an article titled "untersuchungen über den lichtwechsel von ε aurigae" (investigations of the light changes of epsilon aurigae), where he suggested the star was an algol variable and an eclipsing binary.

Russian

В 1904 он издал в "astronomische nachrichten" статью под названием "untersuchungen über den lichtwechsel von ε aurigae" ("Исследования небольших изменений яркости ε Возничего"), где предположил, что звезда является затменной переменной типа Алголя и состоит из двух компонентов.

Last Update: 2016-03-03
Usage Frequency: 1
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Reference: Wikipedia
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