Variability as a Predictor for the Hard-to-soft State Transition in GX 339−4

During the outbursts of black hole X-ray binaries (BHXRBs), their accretion flows transition through several states. The source luminosity rises in the hard state, dominated by nonthermal emission, before transitioning to the blackbody-dominated soft state. As the luminosity decreases, the source tr...

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Detalles Bibliográficos

Principais autores:	Matteo Lucchini, Marina Ten Have, Jingyi Wang, Jeroen Homan, Erin Kara, Oluwashina Adegoke, Riley Connors, Thomas Dauser, Javier Garcia, Guglielmo Mastroserio, Adam Ingram, Michiel van der Klis, Ole König, Collin Lewin, Labani Mallick, Edward Nathan, Patrick O’Neill, Christos Panagiotou, Joanna Piotrowska, Phil Uttley
Formato:	Artigo
Idioma:	Inglês
Publicado:	IOP Publishing 2023-01-01
Series:	The Astrophysical Journal
Assuntos:	Stellar mass black holes Relativistic binary stars Accretion
Acceso en liña:	https://doi.org/10.3847/1538-4357/ad0294
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