Lorentz Factors of Compact Jets in Black Hole X-Ray Binaries

Compact, continuously launched jets in black hole X-ray binaries (BHXBs) produce radio to optical/IR synchrotron emission. In most BHXBs, an IR excess (above the disk component) is observed when the jet is present in the hard spectral state. We investigate why some BHXBs have prominent IR excesses a...

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Veröffentlicht in:	The Astrophysical journal 2019-12, Vol.887 (1), p.21
Hauptverfasser:	Saikia, Payaswini, Russell, David M., Bramich, D. M., Miller-Jones, James C. A., Baglio, Maria Cristina, Degenaar, Nathalie
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Amplitudes Astrophysics Black holes Emission High energy astrophysics Inclination angle Infrared astronomy Infrared excess Jets Lorentz factor Near infrared astronomy Power law Recovery Relativism Relativistic effects Relativistic jets Stellar mass black holes X ray binaries X ray stars
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