Accretion Flow Properties of EXO 1846-031 during Its Multi-peaked Outburst after Long Quiescence

We study the recent outburst of the black hole candidate EXO 1846-031, which went into an outburst in 2019 after almost 34 yr in quiescence. We use archival data from the Swift/XRT, MAXI/GSC, NICER/XTI, and NuSTAR/FPM satellites/instruments to study the evolution of the spectral and temporal propert...

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Auteurs principaux:	Sujoy Kumar Nath, Dipak Debnath, Kaushik Chatterjee, Riya Bhowmick, Hsiang-Kuang Chang, Sandip K. Chakrabarti
Format:	Artigo
Langue:	Inglês
Publié:	IOP Publishing 2023-01-01
Collection:	The Astrophysical Journal
Sujets:	Accretion Black holes Black hole physics X-ray binary stars X-ray transient sources
Accès en ligne:	https://doi.org/10.3847/1538-4357/ad0735
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