A phenomenological model for the X-ray spectrum of nova V2491 Cygni (2012)
Attributed to:
Galaxy formation and evolution 2010 - 2015
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201117835
Publication URI: http://dx.doi.org/10.1051/0004-6361/201117835
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics