A physical model for the continuum variability and quasi-periodic oscillation in accreting black holes Physical PSD model (2011)
Attributed to:
Super-Eddington accretion and ultraluminous X-ray sources
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2011.18860.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2011.18860.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3