Optical spectrum of HDE 245770 and an X-ray flare of the transient source A0535+26.
Abstract
Spectrograms of the Be star HDE 245770, the optical counterpart of the transient X-ray source AO535 + 26, are presented. The spectrograms were obtained over a three-year period using the stellar spectrograph attached to the 6-meter telescope at the Special Astrophysical Observatory in Nizhni Arkhyz, USSR. The dispersion of the spectrograph was 9, 14, and 28 A/mm. A comprehensive list of the lines observed in the range 3450-7000 A is given, and measurements of the principal stellar parameters are provided in a table. Evidence of variability in the spectrum of HDE 245770 is discussed, with emphasis given to an abrupt change occurring around January 1981.
- Publication:
-
Astronomicheskii Zhurnal
- Pub Date:
- April 1985
- Bibcode:
- 1985AZh....62...70A
- Keywords:
-
- B Stars;
- Stellar Spectrophotometry;
- Visible Spectrum;
- X Ray Binaries;
- Line Spectra;
- Spectrum Analysis;
- Astrophysics