Strong disk winds traced throughout outbursts in black-hole X-ray binaries
Author:
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/nature25159.pdf
Reference52 articles.
1. Hirose, S., Blaes, O., Krolik, J., Coleman, M. & Sano, T. Convection causes enhanced magnetic turbulence in accretion disks in outburst. Astrophys. J. 787, 1 (2014)
2. Coleman, M., Kotko, I., Blaes, O., Lasota, J.-P. & Hirose, S. Dwarf nova outbursts with magnetorotational turbulence. Mon. Not. R. Astron. Soc. 462, 3710–3726 (2016)
3. Scepi, N., Lesur, G., Dubus, G. & Flock, M. Impact of convection and resistivity on angular momentum transport in dwarf novae. Astron. Astrophys. https://doi.org/10.1051/0004-6361/201731900 (2017)
4. Kotko, I. & Lasota, J.-P. The viscosity parameter and the properties of accretion disc outbursts in close binaries. Astron. Astrophys. 545, A115 (2012)
5. Lesur, G., Ferreira, J. & Ogilvie, G. I. The magnetorotational instability as a jet launching mechanism. Astron. Astrophys. 550, A61 (2013)
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