Be-Phenomenon in Neutron Star X-ray Binaries
No Thumbnail Available
Links to Files
Permanent Link
Author/Creator ORCID
Date
2017
Type of Work
Department
Program
Citation of Original Publication
Kühnel, M., et al. "Be-Phenomenon in Neutron Star X-ray Binaries." The B[e] Phenomenom: Forty Years of Studies 508 (2017): 385. http://aspbooks.org/custom/publications/paper/508-0385.html.
Rights
This item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
Abstract
In this work we provide a brief insight into two aspects of Be/X-ray binaries, which are probably involved in production of X-ray outbursts: the evolution of the Be star disk, in particular of its size, and the binary geometry which drives gravitational interaction. Simultaneous X-ray and optical data will aid our investigation of the evolution of Be stars in binaries and the X-ray outburst mechanism.