Nova V351 Puppis 1991: A multiwavelength study of the nebular phase

Monthly Notices of the Royal Astronomical Society

Volumn 279, Issue 1, 1996, Pages 280-292

  Saizar, P ^a   Pachoulakis, I ^a   Shore, S N ^b   Starrfield, S ^c   Williams, R E ^d   Rothschild, E ^a   Sonneborn, G ^e  

^a UNIVERSITY OF PENNSYLVANIA   (United States)

^b INDIANA UNIVERSITY SOUTH BEND   (United States)

^c ARIZONA STATE UNIVERSITY   (United States)

^d AURA for the European Space Agency   (United States)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Novae, cataclysmic variables; Stars: individual: Nova Puppis 1991; Ultraviolet: stars

Indexed keywords

GROUND BASED; MULTI-WAVELENGTH STUDY; NOVAE CATACLYSMIC VARIABLES; OPTICAL-; PHYSICAL CONDITIONS; RECOMBINATION LINES; STAR: INDIVIDUAL: NOVA PUPPI 1991; STARS: INDIVIDUAL: PROXIMA CENTAURI; ULTRAVIOLET: STARS; UV-LIGHT;

WHITE DWARFS;

EID: 0008670384     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/279.1.280     Document Type: Article

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