The re-analysis of the ROSAT data of Nova Mus 1983 using white dwarf atmosphere emission models

Monthly Notices of the Royal Astronomical Society

Volumn 326, Issue 4, 2001, Pages 1441-1447

  Balman, S ^a   Krautter, J ^b  

^a MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^b UNIVERSITÄT HEIDELBERG   (Germany)

Author keywords

Atmospheres binaries; Close stars; GQ Muscae stars; Individual; Mass loss novae, cataclysmic variables X rays; Stars

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; TEMPERATURE; X RAY OPTICS; X RAY SCATTERING;

ATMOSPHERE - BINARY; CLASSICAL NOVAE; CLOSE - STAR; DWARF ATMOSPHERES; EMISSION MODEL; GQ MUSCA - STAR; INDIVIDUAL; MASS LOSS; MASS-LOSS - NOVA, CATACLYSMIC VARIABLE - X-RAY; NOVAE CATACLYSMIC VARIABLES;

WHITE DWARFS;

EID: 0010994620     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2001.04716.x     Document Type: Article

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