The interaction of young massive stars with their environment A millimeter and submillimeter line study of NGC 6334 FIR II

Astronomy and Astrophysics

Volumn 465, Issue 3, 2007, Pages 887-898

  Zhang, J S ^a,b,c   Henkel, C ^a   Mauersberger, R ^d   Chin, Y N ^e   Menten, K M ^a   Tieftrunk, A R ^f   Belloche, A ^a  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b CHINESE ACADEMY OF SCIENCES   (China)

^c GUANGZHOU UNIVERSITY   (China)

^d Institute de Radioastronomie Millimétrique IRAM Núcleo Central   (Spain)

^e TAMKANG UNIVERSITY   (Taiwan)

^f Im Acker 21B   (Germany)

Author keywords

ISM: abundances; ISM: atoms; ISM: H II regions; ISM: individual objects: NGC 6334 FIR II; ISM: molecules; Radio lines: ISM

Indexed keywords

GALAXIES; INFRARED RADIATION; MATHEMATICAL MODELS; OXYGEN; PHOTONS; TELESCOPES;

ISM: ABUNDANCES; ISM: ATOMS; ISM: H II REGIONS; ISM: INDIVIDUAL OBJECTS: NGC 6334 FIR II; ISM: MOLECULES; RADIO LINES: ISM;

ASTROPHYSICS;

EID: 34247182670     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065931     Document Type: Article

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