Constraints on star formation theories from the Serpens molecular cloud and protocluster

Astronomy and Astrophysics

Volumn 392, Issue 3, 2002, Pages 1053-1068

  Olmi, L ^a,b,c   Testi, L ^d  

^a UNIVERSITY OF MASSACHUSETTS   (United States)

^b UNIVERSITY OF PUERTO RICO   (Puerto Rico)

^c CNR   (Italy)

^d INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

ISM: Molecules; Radio lines: ISM; Stars: Formation

Indexed keywords

BOLOMETERS; RADIOACTIVE TRACERS; SPACE RESEARCH;

MOLECULAR CLOUDS;

ASTROPHYSICS;

EID: 0036740615     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20020959     Document Type: Article

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