Probing the initial conditions of high-mass star formation: II. Fragmentation, stability, and chemistry towards high-mass star-forming regions G29.96-0.02 and G35.20-1.74

Astronomy and Astrophysics

Volumn 530, Issue , 2011, Pages

  Pillai, T ^a,b,b   Kauffmann, J ^b,c,d   Wyrowski, F ^e   Hatchell, J ^f   Gibb, A G ^g   Thompson, M A ^h  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c HARVARD UNIVERSITY   (United States)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^f UNIVERSITY OF EXETER   (United Kingdom)

^g UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^h UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

Author keywords

Astrochemistry; ISM: clouds; ISM: jets ond outflows; ISM: molecules; Molecular data; Turbulence

Indexed keywords

DEUTERIUM; FIGHTER AIRCRAFT; TURBULENCE;

ASTROCHEMISTRY; ISM : CLOUDS; ISM: JETS OND OUTFLOWS; ISM: MOLECULES; MOLECULAR DATA;

GIANT STARS;

EID: 79957531802     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015899     Document Type: Article

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