Quantitative analysis of WC stars: Constraints on neon abundances from ISO-SWS spectroscopy

Monthly Notices of the Royal Astronomical Society

Volumn 315, Issue 2, 2000, Pages 407-422

  Dessart, Luc ^a,e   Crowther, Paul A ^a   John Hillier, D ^b   Willis, Allan J ^a   Morris, Patrick W ^c,d,f   Van Der Hucht, Karel A ^d  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF PITTSBURGH   (United States)

^c UNIVERSITY OF AMSTERDAM   (Netherlands)

^d SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^e UNIVERSITÉ LAVAL   (Canada)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Infrared: stars; Stars: abundances; Stars: evolution; Stars: fundamental parameters; Stars: Wolf Rayet

Indexed keywords

COSMIC RAYS; COSMOLOGY; STARS;

FINE STRUCTURES; INFRARED: STAR; MIDINFRARED; NONLOCAL; STAR: EVOLUTION; STARS ABUNDANCES; STARS: BE; STARS: WOLF-RAYET; STARS:FUNDAMENTAL PARAMETERS; STELLAR PARAMETERS;

NEON;

EID: 1542633148     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03399.x     Document Type: Article

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