Английская Википедия:29 Aquarii
Шаблон:Short description Шаблон:Starbox begin Шаблон:Starbox image Шаблон:Starbox observe Шаблон:Starbox character Шаблон:Starbox astrometry Шаблон:Starbox orbit Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox end
29 Aquarii is a binary star system located around 590 light years away from the Sun in the equatorial constellation of Aquarius. 29 Aquarii is the Flamsteed designation; the system also bears the variable star designation DX Aquarii. It is a challenge to view with the naked eye, appearing as a dim star with a combined apparent visual magnitude of 6.39.[1] The system is moving further from the Earth with a heliocentric radial velocity of about +15 km/s.[1]
This is a spectroscopic binary system with a close circular orbit taking just 0.945 days to complete.[2] Despite their proximity, this does not appear to be a contact binary system.[3] The orbital plane of the two stars lies near the line of sight, so they form an Algol-type eclipsing binary. The first component of the system is an A-type main sequence star with a stellar classification of A2 V. Its companion is giant star with a classification of K0 III.[4]
The variability of this system was first noticed in 1965 by W. Strohmeier of Remeis-Observatory in Bamberg, Germany.[5] He later discovered that the variability was caused by a binary companion eclipsing the primary star.[6]
References
External links
- ↑ 1,0 1,1 Ошибка цитирования Неверный тег
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; для сносокAnderson2012
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; для сносокPaffhausen1976
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; для сносокRucinski2002
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; для сносокaj138_2_664
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; для сносокStrohmeier1965
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; для сносокStrohmeier1966
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- Английская Википедия
- A-type main-sequence stars
- K-type giants
- Spectroscopic binaries
- Algol variables
- Aquarius (constellation)
- Durchmusterung objects
- Flamsteed objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Bright Star Catalogue objects
- Objects with variable star designations
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