Chemical differentiation in regions of high-mass star formation CS, dust, and N2H+ in southern sources

Astronomy and Astrophysics

Volumn 461, Issue 2, 2007, Pages 523-535

  Pirogov, L ^a   Zinchenko, I ^a,b,c   Caselli, P ^d,e   Johansson, L E B ^f  

^a INSTITUTE OF APPLIED PHYSICS   (Russian Federation)

^b LOBACHEVSKY STATE UNIVERSITY OF NIZHNY NOVGOROD   (Russian Federation)

^c UNIVERSITY OF HELSINKI   (Finland)

^d INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

Author keywords

ISM: clouds; ISM: molecules; Radio lines: ISM; Stars: formation

Indexed keywords

ASTROPHYSICS; DUST; MOLECULAR DYNAMICS; NITROGEN COMPOUNDS; PARAMETER ESTIMATION; PHYSICAL PROPERTIES;

ISM: CLOUDS; ISM: MOLECULES; RADIO LINES: ISM; STARS: FORMATION;

GALAXIES;

EID: 33846341775     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054777     Document Type: Article

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