Evolution of the Accretion Disk and Corona during the Outburst of the Neutron Star Transient MAXI J1807+132

Low-mass X-ray binaries with a neutron star as the primary object show a complex array of phenomenology during outbursts. The observed variability in X-ray emission primarily arises from changes in the innermost regions of the accretion disk, neutron star surface, and corona. In this work, we presen...

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Bibliographic Details
Main Authors: Sandeep K. Rout, Teo Muñoz-Darias, Jeroen Homan, Montserrat Armas Padilla, David M. Russell, Kevin Alabarta, Payaswini Saikia
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ad919f
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