A multiwavelength study of the S106 region III. the S106 molecular cloud as part of the Cygnus X cloud complex

Astronomy and Astrophysics

Volumn 474, Issue 3, 2007, Pages 873-882

  Schneider, N ^a,d   Simon, R ^d   Bontemps, S ^b   Comeron F ^c   Motte, F ^a  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b OBSERVATOIRE DE BORDEAUX   (France)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d UNIVERSITY OF COLOGNE   (Germany)

Author keywords

ISM: clouds; ISM: individual objects: S106; ISM: kinematics and dynamics; ISM: molecules; Radio lines: ISM

Indexed keywords

CORRELATION METHODS; HIGH FREQUENCY TELECOMMUNICATION LINES; LUMINANCE; MOLECULAR STRUCTURE; SATELLITES; ULTRAVIOLET RADIATION;

BIPOLAR NEBULA S106; CYGNUS X CLOUDS; MOLECULAR CLOUDS; MULTIWAVELENGTH;

CLOUDS;

EID: 36049047019     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20077540     Document Type: Article

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