Research Article
Year 1987,
Volume: 36 , - , 01.01.1987
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.
References
- Communications, Series A2-A3: Physical Sciences and Engineering
Year 1987,
Volume: 36 , - , 01.01.1987
Abstract
References
- Communications, Series A2-A3: Physical Sciences and Engineering
There are 1 citations in total.
Details
| Primary Language | English |
|---|---|
| Subjects | Engineering |
| Journal Section | Research Article |
| Authors | |
| Submission Date | January 1, 1987 |
| Publication Date | January 1, 1987 |
| Published in Issue | Year 1987 Volume: 36 |
Cite
Communications Faculty of Sciences University of Ankara Series A2-A3 Physical Sciences and Engineering licensed under a Creative Commons Attribution 4.0 International License.
