The G9.62+0.19-F hot molecular core the infrared view on very young massive stars

Astronomy and Astrophysics

Volumn 429, Issue 3, 2005, Pages 903-921

  Linz, H ^a,b   Stecklum, B ^a   Henning, Th ^b   Hofner, P ^c,d   Brandl, B ^e,f  

^a THÜRINGER LANDESSTERNWARTE TAUTENBURG   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c NEW MEXICO INSTITUTE OF MINING AND TECHNOLOGY   (United States)

^d NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^e Cornell University ^*  (United States)

^f LEIDEN UNIVERSITY   (Netherlands)

Author keywords

Circumstellar matter infrared; Dust, extinction ISM; Formation stars; G9.62+0.19; Individual objects; Stars; Stars ISM

Indexed keywords

COMPUTATIONAL COMPLEXITY; DATA REDUCTION; DUST; INFRARED RADIATION; LIGHT EMISSION; MATHEMATICAL MODELS;

INFRARED:STARS; ISM:DUST; ISM:EXTINCTION; ISM:INDIVIDUAL OBJECTS:G9.62+0.19; MOLECULAR CORE; STARS:CIRCUMSTELLAR MATTER; STARS:FORMATION;

ASTRONOMY;

EID: 11844278540     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:200400035     Document Type: Review

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