<i>IXPE</i> View of BH XRBs during the First 2.5 Years of the Mission

<i>IXPE</i> View of BH XRBs during the First 2.5 Years of the Mission

Accreting stellar-mass black holes represent unique laboratories for studying matter and radiation under the influence of extreme gravity. They are highly variable sources going through different accretion states, showing various components in their X-ray spectra from the thermal emission of the acc...

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Bibliographic Details
Main Authors: Michal Dovčiak, Jakub Podgorný, Jiří Svoboda, James F. Steiner, Philip Kaaret, Henric Krawczynski, Adam Ingram, Vadim Kravtsov, Lorenzo Marra, Fabio Muleri, Javier A. García, Guglielmo Mastroserio, Romana Mikušincová, Ajay Ratheesh, Nicole Rodriguez Cavero
Format: Article
Language:English
Published: MDPI AG 2024-09-01
Series:Galaxies
Subjects:
X-ray polarisation
high-energy processes
black holes
X-ray binaries
Online Access:https://www.mdpi.com/2075-4434/12/5/54

Internet

https://www.mdpi.com/2075-4434/12/5/54

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