Molecular and atomic gas in the large magellanic cloud. II. Three-dimensional correlation between CO and I

Astrophysical Journal

Volumn 705, Issue 1, 2009, Pages 144-155

  Fukui, Y ^a   Kawamura, A ^a   Wong, T ^b   Murai, M ^a   Iritani, H ^a   Mizuno, N ^a,c   Mizuno, Y ^a   Onishi, T ^a,d   Hughes, A ^e,f   Ott, J ^g,h   Muller, E ^a   Staveley Smith, L ⁱ   Kim, S ^j  

^a NAGOYA UNIVERSITY   (Japan)

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

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^d Osaka Prefecture University   (Japan)

^e SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^f CSIRO   (Australia)

^g NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ UNIVERSITY OF WESTERN AUSTRALIA   (Australia)

^j Sejong University   (South Korea)

more..

Author keywords

Galaxies: ISM; ISM: atoms; ISM: clouds; ISM: molecules; Magellanic Clouds; Radio lines: ISM

Indexed keywords

EID: 70549110033     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/705/1/144     Document Type: Article

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