One Hundred Years of Observations of the Be Star HDE 245770 (the X-ray Binary A0535+26/V725 Tau): The End of an Active Phase
arXiv:astro-ph/0007321 · doi:10.1134/1.20364
Abstract
UBV observations of the X-ray binary system A0535+26/V725 Tau at the Crimean Station of the Sternberg Astronomical Institute in 1980-1998 are presented. Based on our and published data, we analyze the photometric history of the star from 1898.
Translated from Pis'ma Astronomicheskii Zhurnal, Vol. 26, No. 1, 2000, pp. 13-26
Cited by in corpus (9)
- The gas-to-extinction ratio and the gas distribution in the Galaxy
- Distances to Galactic X-ray Binaries with Gaia DR2
- Joint H-alpha and X-Ray Observations of Massive X-Ray Binaries. III. The Be X-ray Binaries HDE 245770 = A 0535+26 and X Persei
- Cyclical behaviour and disc truncation in the Be/X-ray binary A0535+26
- Long-term variability of high-mass X-ray binaries. I.Photometry
- Discrete Mass Ejections from the Be/X-ray Binary A0535+26/HD245770
- X-ray spectral-timing variability of 1A 0535+262 during the 2020 giant outburst
- Time delay between the optical and X-ray outbursts in the high mass X-ray transient A0535+26/HDE245770
- Further evidence for natal kick segregation by spectral type in high-mass X-ray binaries