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Detection of the progenitors of Be X-ray Binaries

Published online by Cambridge University Press:  30 December 2019

Douglas Gies Open the ORCID record for Douglas Gies [Opens in a new window] ,
Luqian Wang Open the ORCID record for Luqian Wang [Opens in a new window]  and
Geraldine Peters
Douglas Gies
Affiliation:
CHARA, Dept. of Physics & Astronomy, Georgia State University, P.O. Box 5060, Atlanta, GA 30302-5060, USA emails: gies@chara.gsu.edu, lwang@chara.gsu.edu
Luqian Wang
Affiliation:
CHARA, Dept. of Physics & Astronomy, Georgia State University, P.O. Box 5060, Atlanta, GA 30302-5060, USA emails: gies@chara.gsu.edu, lwang@chara.gsu.edu
Geraldine Peters
Affiliation:
Space Sciences Center, University of Southern California, Los Angeles, CA 90089-1341, USA email: gpeters@usc.edu
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Abstract

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A recent survey of the far-ultraviolet spectra of 264 B-emission line stars has revealed 16 systems with hot companions that are the stripped down remains of a former mass donor star. Some of these will probably become Be + neutron star X-ray binaries in the future. The actual numbers of such systems may be large, because the detected systems have companions that occupy the brief and bright, He-shell burning stage of evolution.

Keywords

binaries: spectroscopicstars: emission-line Bestars: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 143 - 145
Copyright
© International Astronomical Union 2019 

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