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  • Communications Faculty of Sciences University Ankara Series A2-A3 Physical and Engineering
  • Volume:36
  • HD 167971:A Bright Massive Close Eclipsing System

HD 167971:A Bright Massive Close Eclipsing System

Authors : Osman DEMİRCAN
Pages : 0-0
Doi:10.1501/commua1-2_0000000070
View : 40 | Download : 9
Publication Date : 1987-01-01
Article Type : Research Paper
Abstract :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.
Keywords : HD 167971, Binary, System

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