W43: The closest molecular complex of the Galactic bar?

Astronomy and Astrophysics

Volumn 529, Issue , 2011, Pages

  Nguyen Lu'o'ng Q ^a   Motte, F ^a   Schuller, F ^b   Schneider, N ^a   Bontemps, S ^c   Schilke, P ^d   Menten, K M ^b   Heitsch, F ^e   Wyrowski, F ^b   Carlhoff, P ^d   Bronfman, L ^f   Henning, T ^g  

^a CEA SACLAY   (France)

^b MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^c LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

^d UNIVERSITY OF COLOGNE   (Germany)

^e The University of North Carolina at Chapel Hill   (United States)

^f UNIVERSITY OF CHILE   (Chile)

^g MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

dust, extinction; HII regions; ISM: clouds; ISM: kinematics and dynamics; stars: formation; submillimeter: ISM

Indexed keywords

DUST , EXTINCTION; HII REGIONS; ISM : CLOUDS; ISM: KINEMATICS AND DYNAMICS; STARS: FORMATION; SUBMILLIMETER: ISMS;

ATOMS; CLOUDS; DENSITY OF GASES; DUST; GALAXIES; GASES; KINEMATICS; MOLECULAR SPECTROSCOPY; SURVEYS;

STARS;

EID: 79953169463     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016271     Document Type: Article

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