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The spectroscopic evolution of the symbiotic-like recurrent nova V407 Cygni during its 2010 outburst
- 1.0367909 - ASÚ 2012 RIV FR eng J - Journal Article
Shore, S. N. - Wahlgren, G.M. - Augusteijn, T. - Liimets, T. - Page, K.L. - Osborne, J.P. - Beardmore, A.P. - Koubský, Pavel - Šlechta, Miroslav - Votruba, Viktor
The spectroscopic evolution of the symbiotic-like recurrent nova V407 Cygni during its 2010 outburst.
Astronomy & Astrophysics. Roč. 527, March (2011), A98/1-A98/15. ISSN 0004-6361. E-ISSN 1432-0746
Grant - others:EU(XE) ESA PECS project No 98058.
Institutional research plan: CEZ:AV0Z10030501
Keywords : novae * cataclysmic variables
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 4.587, year: 2011
Unlike classical novae occurring in compact cataclysmic binary systems, for which the ejecta undergo free ballistic expansion, the explosion of nova V407 Cyg occurred within the dense, complex wind of a Mira variable companion. This paper concentrates on the development of the shock and its passage through the Mira wind. We also present some constraints on the binary system properties.
Permanent Link: http://hdl.handle.net/11104/0202418
Number of the records: 1