On the internal structure of starless cores I. Physical conditions and the distribution of CO, CS, N2H+, and NH3 in L1498 and L1517B

Astronomy and Astrophysics

Volumn 416, Issue 1, 2004, Pages 191-212

  Tafalla, M ^a   Myers, P C ^b   Caselli, P ^c   Walmsley, C M ^c  

^a OBSERVATORIO ASTRONÓMICO NACIONAL   (Spain)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

ISM: abundances; ISM: clouds; ISM: individual objects: L1498, L1517B; ISM: molecules; Stars: formation

Indexed keywords

APPROXIMATION THEORY; ATMOSPHERIC COMPOSITION; ATMOSPHERIC DENSITY; ATMOSPHERIC RADIATION; ATMOSPHERIC TURBULENCE; EXTRATERRESTRIAL ATMOSPHERES; MONTE CARLO METHODS;

INTERNAL STRUCTURE; INTERSTELLAR MEDIUM; ISOTHERMAL SPHERES; STARLESS CORES;

ATMOSPHERIC CHEMISTRY;

EID: 1542436796     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031704     Document Type: Article

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