WR 7a: A V Sagittae or a qWR star?

Monthly Notices of the Royal Astronomical Society

Volumn 346, Issue 3, 2003, Pages 963-967

  Oliveira, A S ^a   Steiner, J E ^a   Cieslinski, D ^b  

^a UNIVERSITY OF SÃO PAULO   (Brazil)

^b INSTITUTO NACIONAL DE PESQUISAS ESPACIAIS   (Brazil)

Author keywords

Stars: emission line, Be; Stars: fundamental parameters; Stars: individual: WR 7a; Stars: Wolf Rayet

Indexed keywords

ABSORPTION SPECTROSCOPY; PHOTOMETRY;

INTENSITY SPECTRUM; NOISE LEVELS; OPTICAL-; SPECTRA'S; STAR: INDIVIDUAL: WR 7A; STARS: EMISSION-LINE BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: WOLF-RAYET; STARS:FUNDAMENTAL PARAMETERS; TEMPORAL VARIANCE;

STARS;

EID: 0348158202     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2003.07157.x     Document Type: Article

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