The spectroscopic evolution of the symbiotic-like recurrent nova V407 Cygni during its 2010 outburst: II. the circumstellar environment and the aftermath

Astronomy and Astrophysics

Volumn 540, Issue , 2012, Pages

  Shore, S N ^a,b   Wahlgren, G M ^c,d   Augusteijn, T ^e   Liimets, T ^e,f   Koubsky, P ^g   Slechta M ^g   Votruba, V ^g  

^a UNIVERSITY OF PISA   (Italy)

^b INFN SEZIONE DI PISA   (Italy)

^c CATHOLIC UNIVERSITY OF AMERICA   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e NORDIC OPTICAL TELESCOPE   (Spain)

^f TARTU OBSERVATORY   (Estonia)

^g ASTRONOMICAL INSTITUTE   (Czech Republic)

Author keywords

binaries: symbiotic; gamma ray burst: general; novae, cataclysmic variables; stars: individual: V407 Cygni

Indexed keywords

IONIZATION; STARS;

BINARIES: SYMBIOTIC; CIRCUMSTELLAR; GAMMA-RAY BURST: GENERALS; HIGH RESOLUTION; LOW-VELOCITY; NOVAE CATACLYSMIC VARIABLES; SPECTROSCOPIC EVOLUTION; STAR: INDIVIDUAL: V407 CYGNI; STARS: INDIVIDUAL: PROXIMA CENTAURI;

GAMMA RAYS;

EID: 84859042758     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118060     Document Type: Article

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