A phenomenological model for the X-ray spectrum of nova V2491 Cygni (2012)

First Author: Pinto C
Attributed to:  IoA Theoretical and X-ray Astronomy consolidation 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