Observations of the Disk/Jet Coupling of MAXI J1820+070 during Its Descent to Quiescence

Black hole X-ray binaries in the quiescent state (Eddington ratios typically 10−5) display softer X-ray spectra (photon indices Γ ∼ 2) compared to higher-luminosity black hole X-ray binaries in the hard state (Γ ∼ 1.7). However, the cause of this softening and its implications for the underlying acc...

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Veröffentlicht in:	The Astrophysical journal 2021-01, Vol.907 (1), p.34
Hauptverfasser:	Shaw, A. W., Plotkin, R. M., Miller-Jones, J. C. A., Homan, J., Gallo, E., Russell, D. M., Tomsick, J. A., Kaaret, P., Corbel, S., Espinasse, M., Bright, J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Astrophysics Black holes Decay Deposition Emission Low-mass x-ray binary stars Luminosity Physics Radio spectra Sciences of the Universe Softening Spectrum allocation Synchrotrons X ray binaries X ray spectra X ray stars X-ray emissions X-ray transient sources X-rays
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