Strong disk winds traced throughout outbursts in black-hole X-ray binaries

Analysis of the light curves of outbursts in black-hole X-ray binaries suggests that throughout the accretion process mass is lost from the accretion disks through strong, magnetically driven disk winds. Windy disks Black holes, neutron stars and white dwarfs in close binary systems where mass is fl...

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Veröffentlicht in:	Nature (London) 2018-02, Vol.554 (7690), p.69-72
Hauptverfasser:	Tetarenko, B. E., Lasota, J.-P., Heinke, C. O., Dubus, G., Sivakoff, G. R.
Format:	Artikel
Sprache:	eng
Schlagworte:	639/33/34/864 639/766/34/864 Accretion disks Angular momentum Bayesian analysis Binary stars Black holes Black holes (Astronomy) Humanities and Social Sciences Instability letter Light Magnetic fields Mass transport Mathematical models Momentum transport multidisciplinary Neutron stars Numerical simulations Observations Parameter estimation Physics Science Stars & galaxies Stellar evolution Viscosity White dwarf stars Wind Winds X ray binaries X ray stars
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