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The spectroscopic evolution of the symbiotic-like recurrent nova V407 Cygni during its 2010 outburst
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SYSNO ASEP 0367909 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title The spectroscopic evolution of the symbiotic-like recurrent nova V407 Cygni during its 2010 outburst Author(s) Shore, S. N. (IT)
Wahlgren, G.M. (US)
Augusteijn, T. (ES)
Liimets, T. (ES) ORCID
Page, K.L. (GB)
Osborne, J.P. (GB)
Beardmore, A.P. (GB)
Koubský, Pavel (ASU-R) RID, ORCID
Šlechta, Miroslav (ASU-R) RID, ORCID
Votruba, Viktor (ASU-R) RIDSource Title Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 527, March (2011), A98/1-A98/15Number of pages 15 s. Language eng - English Country FR - France Keywords novae ; cataclysmic variables Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000287484100113 DOI 10.1051/0004-6361/201015901 Annotation 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. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2012
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