The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst: I. the optically thick phase and the origin of moving lines in novae

Astronomy and Astrophysics

Volumn 533, Issue , 2011, Pages

  Shore, S N ^a   Augusteijn, T ^b   Ederoclite, A ^c,d   Uthas, H ^e  

^a UNIVERSITY OF PISA   (Italy)

^b NORDIC OPTICAL TELESCOPE   (Spain)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^d UNIVERSIDAD DE LA LAGUNA   (Spain)

^e Columbia University ^*  (United States)

Author keywords

Cataclysmic variables; Novae; Stars: individual: T Pyx

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; SODIUM COMPOUNDS; SPECTROSCOPIC ANALYSIS;

ABSORPTION FEATURES; ABSORPTION LINES; CATACLYSMIC VARIABLES; DIFFUSE ABSORPTIONS; EMISSION LINES; HIGH-RESOLUTION SPECTROSCOPY; NOVA; SPECTROSCOPIC EVOLUTION; STAR: INDIVIDUAL: T PYX; STARS: INDIVIDUAL: PROXIMA CENTAURI;

STARS;

EID: 80052194781     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117721     Document Type: Article

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