Abundance analysis of the slow nova PW Vulpeculae 1984

Monthly Notices of the Royal Astronomical Society

Volumn 290, Issue 1, 1997, Pages 75-86

  Schwarz, Greg J ^a  

^a ARIZONA STATE UNIVERSITY   (United States)

Author keywords

Novae, cataclysmic variables; Stars: Abundances; Stars: Individual: PW Vul

Indexed keywords

ELECTRON TEMPERATURE; PHOTOIONIZATION; STARS;

ABUNDANCE ANALYSIS; ELEMENTAL ABUNDANCE; EMISSION LINES; MINIMISATION; NOVAE CATACLYSMIC VARIABLES; PHOTOIONIZATION MODELS; STAR: INDIVIDUAL: PW VUL; STARS ABUNDANCES; STARS: INDIVIDUAL: PROXIMA CENTAURI; ULTRA-VIOLET SPECTRUMS;

ELECTROMAGNETIC WAVE EMISSION;

EID: 0002121059     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/290.1.75     Document Type: Article

References (2)

1. Austin S. J., Wagner R. M., Starrfield S., Shore S. N., Sonneborn G., Bertram R., 1996, AJ, 111, 869
2. Bohlin R. C., Sparks W. M., Holm A. V., Savage B. D., Snijders M. A. J., 1980, A&A, 85, 1