Modelling the high-mass accretion rate spectra of GX 339-4: black hole spin from reflection? High-mass accretion in GX 339-4 (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.1365-2966.2011.19040.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2011.19040.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society