HD 206267, a candidate star for the transient X-ray source Cepheus X-4?
Abstract
Summary. The spectrum of the 3.7 day spectroscopic binary HD 206267 shows no evidence for large mass loss. No emission lines could be detected in the wavelength region 37506680 A. The orbital elements of the system suggest a massive secondary which can be interpreted as a normal non-degenerate star. Key words: X-ray sources radial velocities
- Publication:
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Astronomy and Astrophysics
- Pub Date:
- February 1975
- Bibcode:
- 1975A&A....39..157H