Aleksander Sadowski
Published 2009-06-01, updated 2009-10-26Version 2
We investigate stationary slim accretion disks around Kerr black holes. We construct a new numerical method based on the relaxation technique. We systematically cover the whole parameter space relevant to stellar mass X-ray binaries. We also notice some non-monotonic features in the disk structure, overlooked in previous studies.
Comments: 12 pages, 11 figures. The relativistic slim accretion disk solutions have been published online at http://users.camk.edu.pl/as/slimdisk. An appendix containing the manual for the data available online has been added to the previous version of the paper
Journal: Astrophys.J.Supp.183:171-178,2009
Estimation of bipolar jets from accretion discs around Kerr black holes
Magnetocentrifugal launching of jets from disks around Kerr black holes
Polarization Patterns of Non-Circular Hotspots around Kerr Black Holes: A Preliminary Study
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