Stellar disruption by a supermassive black hole: is the light curve really proportional to t -5/3 ? (2009)
Attributed to:
Research in Theoretical Astrophysics: Accretion, Structure and Evolution in Gravitating Systems
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2008.14049.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2008.14049.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1