A combined V light curve of a recently discovered bright massive close eclipsing binary system HD 167971 has been analyzed by Wilson-Dewinney code. Because of a very Iow amplitu- de variation in light, no unique solution for the physical and geometrical elements could be obta- ined. However, evidences are found that the contact or almost contact component stars have comparable masses around 50 Mo each, and the inclination of the orbit is about 65°. There may be a third component star in the system.
Birincil Dil | İngilizce |
---|---|
Konular | Mühendislik |
Bölüm | Research Article |
Yazarlar | |
Yayımlanma Tarihi | 1 Ocak 1987 |
Gönderilme Tarihi | 1 Ocak 1987 |
Yayımlandığı Sayı | Yıl 1987 |
Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering
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