Early post-maximum spectral evolution of the fast novae V4742 Sagittarii and V4743 Sagittarii

Monthly Notices of the Royal Astronomical Society

Volumn 344, Issue 2, 2003, Pages 521-526

  Morgan, G E ^a   Ringwald, F A ^a,b   Prigge, J W ^b  

^a Central Valley Astronomers Incorporated   (United States)

^b CALIFORNIA STATE UNIVERSITY   (United States)

Author keywords

Instrumentation: Miscellaneous; Line: Identification; Methods: Observational; Novae, cataclysmic variables; Stars: Fundamental parameters

Indexed keywords

HELIUM; IRON COMPOUNDS; STARS;

EMISSION LINES; INSTRUMENTATION: MISCELLANEOUS; LIGHT CURVES; LINE:IDENTIFICATION; METHODS:OBSERVATIONAL; NOVAE CATACLYSMIC VARIABLES; SPECTRA'S; SPECTRAL EMISSION; SPECTRAL EVOLUTION; STARS:FUNDAMENTAL PARAMETERS;

ELECTROMAGNETIC WAVE EMISSION;

EID: 0141955853     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06852.x     Document Type: Article

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