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Omicron Andromedae
・ Omicron Aquarii
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・ Omicron Centauri
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・ Omicron Cephei
・ Omicron Columbae
・ Omicron Coronae Borealis


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Omicron Andromedae : ウィキペディア英語版
Omicron Andromedae


Omicron Andromedae (ο And, ο Andromedae) is a star system in the constellation Andromeda. It is approximately 692 light years from Earth.
Omicron Andromedae is a binary star, whose two components are both spectroscopic binaries themselves, making a four-star system. The system as a whole is classified as a blue-white B-type giant with a mean combined apparent magnitude of +3.62.
The separation of the two brightest components, ο Andromedae A and ο Andromedae B, is 0.34 arcseconds. They have an orbital period of 68.6 years. A is separated from its spectroscopic companion by 0.05 arcseconds. A is a Gamma Cassiopeiae type variable star and the system's brightness varies from magnitude +3.58 to +3.78. This, in turn, has made determination the orbital period of A's spectroscopic binary difficult.〔 B's spectroscopic companion was discovered in 1989, and that binary has a period of 33.01 years.〔
This star system has a peculiar velocity of .〔
==References==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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