Results of the ESO-SEST key programme on CO in the Magellanic Clouds. X. CO emission from star formation regions in LMC and SMC

Astronomy and Astrophysics

Volumn 406, Issue 3, 2003, Pages 817-828

  Israel, F P ^a   Johansson, L E B ^b   Rubio, M ^c   Garay, G ^c   De Graauw, Th ^d   Booth, R S ^b   Boulanger, F ^e,f   Kutner, M L ^g   Lequeux, J ^h   Nyman, L A ^b,i  

^a LEIDEN UNIVERSITY   (Netherlands)

^b CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^c UNIVERSITY OF CHILE   (Chile)

^d SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^e ECOLE NORMALE SUPÉRIEURE   (France)

^f UNIVERSITÉ PARIS SUD   (France)

^g The University of Texas at Austin   (United States)

^h OBSERVATOIRE DE PARIS   (France)

ⁱ EUROPEAN SOUTHERN OBSERVATORY   (Chile)

Author keywords

Galaxies: irregular; Galaxies: ISM; Galaxies: local group; Galaxies: Magellanic Clouds; ISM: molecules

Indexed keywords

CARBON MONOXIDE; CLOUDS; DENSIFICATION; GALAXIES; PHOTODISSOCIATION; SOLAR SYSTEM;

ISOTOPIC EMISSION; MAGELLANIC CLOUDS; MOLECULAR CLOUDS; STAR;

ASTROPHYSICS;

EID: 0043202968     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030784     Document Type: Article

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