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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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I tiakina i:
Ngā kaituhi matua: 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
Hōputu: Artigo
Reo:Inglês
I whakaputaina: IOP Publishing 2023-01-01
Rangatū:The Astrophysical Journal
Ngā marau:
Stellar mass black holes
Relativistic binary stars
Accretion
Urunga tuihono:https://doi.org/10.3847/1538-4357/ad0294
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