Forming an early O-type star through gas accretion?

Astronomy and Astrophysics

Volumn 479, Issue 2, 2008, Pages

  Zapata, L A ^a   Palau, A ^b   Ho, P T P ^c,d   Schilke, P ^a   Garrod, R T ^a   Rodriguez L F ^e   Menten, K ^a  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^e INSTITUTO DE MATEMÁTICAS   (Mexico)

Author keywords

ISM: jets and outflows; ISM: molecules; Molecular data; Radio lines: ISM; Stars: formation; Techniques: interferometric

Indexed keywords

CLUSTER ANALYSIS; GAS DYNAMICS; MOLECULAR STRUCTURE; QUENCHING; VELOCITY MEASUREMENT;

ISM: MOLECULES; MOLECULAR DATA; RADIO LINES: ISM; STARS: FORMATION;

STARS;

EID: 39049141043     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078846     Document Type: Article

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