<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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Autors principals:	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:	Artigo
Idioma:	Inglês
Publicat:	MDPI AG 2024-09-01
Col·lecció:	Galaxies
Matèries:	X-ray polarisation high-energy processes black holes X-ray binaries
Accés en línia:	https://www.mdpi.com/2075-4434/12/5/54
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