The P Cygni supergiant [OMN2000] LS1 - Implications for the star formation history of W51

Astronomy and Astrophysics

Volumn 504, Issue 2, 2009, Pages 429-435

  Clark, J S ^a   Davies, B ^b,c   Najarro, F ^d   MacKenty, J ^e   Crowther, P A ^f   Messineo, M ^c   Thompson, M A ^g  

^a OPEN UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF LEEDS   (United Kingdom)

^c ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

^d CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

^e STScI   (United States)

^f UNIVERSITY OF SHEFFIELD   (United Kingdom)

^g UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

Author keywords

Galaxy: Open clusters and associations: general; ISM: HII regions; Stars: early type; Stars: evolution

Indexed keywords

GALAXY: OPEN CLUSTERS AND ASSOCIATIONS: GENERAL; ISM: HII REGIONS; MASSIVE STARS; MONTE CARLO SIMULATION; NEAR-IR SPECTROSCOPY; STAR CLUSTERS; STAR FORMATIONS; STAR-FORMING REGION; STARS: EARLY-TYPE; STARS: EVOLUTION;

COMPUTER SIMULATION; GALAXIES; MONTE CARLO METHODS; THERMAL LOGGING;

STARS;

EID: 70349320316     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911980     Document Type: Article

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