Circumstellar discs in X/gamma-ray binaries: first results from the Echelle spectrograph

Abstract

Here we report our first spectral observations of Be/X-ray and gamma-ray binaries obtained with the new Echelle spectrograph of the National Astronomical Observatory Rozhen. For four objects (LSI+61303, gamma Cas, MWC 148, 4U 2206+54), we report the parameters and estimate the sizes of their circumstellar discs using different emission lines (H-alpha, H-beta, H-gamma, HeI and FeII). For MWC 148, we find that the compact object goes deeply through the disc. The flank inflections of H-alpha can be connected with inner ring formed at the periastron passage or radiation transfer effects. We point out an intriguing similarity between the optical emission lines of the $\gamma$-ray binary MWC 148 and the well known Be star $\gamma$ Cas.

presented at the 10th conference of Astronomical Society of Bulgaria (Belogradchik, 2-5 July 2015); to appear in Blg AJ, v. 24 (2015)

Cited by in corpus (2)

• Optical spectroscopy of Be/gamma-ray binaries
• Mass of the compact object in the Be/gamma-ray binaries LSI+61303 and MWC 148