Spectral evolution of the nova V2468 Cygni: Asymmetric and variable profiles of its emission lines

Astronomy and Astrophysics

Volumn 526, Issue 9, 2011, Pages

  Iijima, T ^a   Naito, H ^b,c  

^a INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^b Nishi Harima Astronomical Observatory   (Japan)

^c NAGOYA UNIVERSITY   (Japan)

Author keywords

novae, cataclysmic variables; stars: individual: V2468 Cygni

Indexed keywords

ASTRONOMICAL OBSERVATORIES; ASTROPHYSICAL OBSERVATORY; CLASSICAL NOVAE; EMISSION LINES; HELIUM ABUNDANCE; NOVAE , CATACLYSMIC VARIABLES; SPECTRAL EVOLUTION; STARS: INDIVIDUAL: V2468 CYGNI;

BUILDINGS; HELIUM; IODINE; OBSERVATORIES; STARS;

ELECTROMAGNETIC WAVE EMISSION;

EID: 78650860722     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015448     Document Type: Article

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