Clustering of emission-line stars in the W 5 e H II region

Publications of the Astronomical Society of Japan

Volumn 60, Issue 4, 2008, Pages 739-748

  Nakano, Makoto ^a   Sugitani, Koji ^b   Niwa, Takahiro ^c   Itoh, Yoichi ^c   Watanabe, Makoto ^d  

^a OITA UNIVERSITY   (Japan)

^b NAGOYA CITY UNIVERSITY   (Japan)

^c KOBE UNIVERSITY   (Japan)

^d NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

ISM: H II regions; ISM: Individual (W 5); Stars: Formation; Stars: Pre main sequence

Indexed keywords

AGGREGATES; BROMINE COMPOUNDS; ELECTROMAGNETIC WAVE EMISSION;

CLUSTERINGS; EMISSION LINES; H II REGIONS; ISM: H II REGIONS; ISM: INDIVIDUAL (W 5); ISM: INDIVIDUALS; PMS STARS; STARS FORMATION; STARS: BE; STARS: PRE-MAIN SEQUENCE;

STARS;

EID: 52049098973     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/60.4.739     Document Type: Article

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