Kühnel, M.Kretschmar, P.Fürst, F.Pottschmidt, KatjaHemphill, P.Rothschild, R. E.Okazaki, A. T.Sagredo, M.Wilms, J.2023-08-312023-08-312017Kühnel, 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.http://hdl.handle.net/11603/29487In 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.en-USThis 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.Be-PhenomenonBe X-ray BinariesX-ray / Hα ConnectionTidal InteractionsText