Optical Properties and Variability of the Be X-Ray Binary CPD-29 2176

Optical Properties and Variability of the Be X-Ray Binary CPD-29 2176

Be X-ray binaries (Be XRBs) are high-mass X-ray binaries, with a neutron star or black hole orbiting and accreting material from a nonsupergiant B-star that is rotating at a near critical rate. These objects are prime targets to understand past binary interactions as the neutron star or black hole p...

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Bibliographic Details
Main Authors: Clarissa M. Pavao, Noel D. Richardson, Jonathan Labadie-Bartz, Herbert Pablo, André-Nicolas Chené
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Be stars
Early-type stars
High mass x-ray binary stars
Binary stars
Circumstellar disks
Stellar oscillations
Online Access:https://doi.org/10.3847/1538-4357/ad07cf

Internet

https://doi.org/10.3847/1538-4357/ad07cf

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