Английская Википедия:50 Persei
Шаблон:Short description Шаблон:Starbox begin Шаблон:Starbox image Шаблон:Starbox observe Шаблон:Starbox character Шаблон:Starbox astrometry Шаблон:Starbox detail Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox end 50 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.52,[1] which is bright enough to be seen with the naked eye. Located around Шаблон:Convert distant, it is a White main-sequence star of spectral type F7V,[2] a star that is currently fusing its core hydrogen. In 1998 the star was named a candidate Gamma Doradus variable with a period of 3.05 days,[3] which would means it displays variations in luminosity due to non-radial pulsations in the photosphere. Subsequently, it was classified as a RS Canum Venaticorum and BY Draconis variable by an automated program.[4]
This is probably a binary system with an unseen companion. It is physically associated with the likely binary system HIP 19255, with the two pairs orbiting each other over a time scale of around a million years. The components of HIP 19255 have an angular separation of 3.87″ and the two components orbit each other every 590 years. 50 Persei may share a gravitational association with Capella, even though the two are separated by nearly 15° − equivalent to a distance of Шаблон:Convert.[5]
50 Persei is emitting an infrared excess at a wavelength of 70 μm, suggesting the presence of a circumstellar debris disk. The disk has a temperature of Шаблон:Val.[6]
References
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- Английская Википедия
- Perseus (constellation)
- Flamsteed objects
- F-type main-sequence stars
- Objects with variable star designations
- RS Canum Venaticorum variables
- Hipparcos objects
- Bright Star Catalogue objects
- Henry Draper Catalogue objects
- Gliese and GJ objects
- BY Draconis variables
- Durchmusterung objects
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