Properties, evolution and morpho-kinematical modelling of the very fast nova V2672 Oph (Nova Oph 2009), a clone of U Sco

Monthly Notices of the Royal Astronomical Society

Volumn 410, Issue 1, 2011, Pages 525-534

  Munari, U ^a,b   Ribeiro, V A R M ^c   Bode, M F ^c   Saguner, T ^a,d  

^a ANS Collaboration   (Italy)

^b C/o Astronomical Observatory ^*  (Italy)

^c LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF PADOVA   (Italy)

Author keywords

Line: profiles; Novae, cataclysmic variables

Indexed keywords

SUPERNOVAE; WHITE DWARFS;

CLASSICAL NOVAE; EXPANSION VELOCITY; GALACTIC CENTER; GALACTOCENTRIC DISTANCES; KINEMATICAL MODELS; LINE OF SIGHT; LINE: PROFILES; LINES-OF-SIGHT; NOVAE CATACLYSMIC VARIABLES; PROPERTY;

LUMINANCE;

EID: 78650122823     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.17462.x     Document Type: Article

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