Molecular line mapping of the giant molecular cloud associated with RCW 106 - II. Column density and dynamical state of the clumps

Monthly Notices of the Royal Astronomical Society

Volumn 386, Issue 2, 2008, Pages 1069-1084

  Wong, T ^a,b,c   Ladd, E F ^d   Brisbin, D ^d,e   Burton, M G ^a   Bains, I ^a,f   Cunningham, M R ^a   Lo, N ^a,c   Jones, P A ^a   Thomas, K L ^g   Longmore, S N ^a,c,h   Vigan, A ^a   Mookerjea, B ^i,j   Kramer, C ⁱ   Fukui, Y ^k   Kawamura, A ^k  

^a UNIVERSITY OF NEW SOUTH WALES   (Australia)

^b UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

^c CSIRO   (Australia)

^d BUCKNELL UNIVERSITY   (United States)

^e Department of Population Medicine and Diagnostic Sciences   (United States)

^f SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^g UNIVERSITY OF KENTUCKY   (United States)

^h HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

ⁱ UNIVERSITY OF COLOGNE   (Germany)

^j TATA INSTITUTE OF FUNDAMENTAL RESEARCH   (India)

^k NAGOYA UNIVERSITY   (Japan)

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Author keywords

ISM: clouds; ISM: molecules; ISM: structure; Stars: formation

Indexed keywords

BINDING ENERGY; DENSITY OF GASES; MAPPING; MASS SPECTROMETRY; OPTICAL PROPERTIES;

COLUMN DENSITY; GIANT MOLECULAR CLOUDS; ISM : CLOUDS; ISM: STRUCTURE; ISM:MOLECULES; LINE MAPPING; MOLECULAR LINES; OPTICAL DEPTH; RCW 106; STARS FORMATION;

CLOUDS;

EID: 42649143249     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13107.x     Document Type: Article

References (57)