Ultraluminous X-ray sources as magnetically powered sub-Eddington advective accretion flows around stellar mass black holes
Author:
Affiliation:
1. Department of Physics, Indian Institute of Science, Bangalore 560012, India
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/482/1/L24/26038571/sly165.pdf
Reference55 articles.
1. An ultraluminous X-ray source powered by an accreting neutron star
2. A highly magnetized twin-jet base pinpoints a supermassive black hole
3. Instability, turbulence, and enhanced transport in accretion disks
4. The Limiting Luminosity of Accreting Neutron Stars With Magnetic Fields
5. Super-Eddington Fluxes from Thin Accretion Disks?
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