The james clerk maxwell telescope nearby galaxies legacy survey. II. Warm molecular gas and star formation in three field spiral galaxies

Astrophysical Journal

Volumn 714, Issue 1, 2010, Pages 571-588

  Warren, B E ^a,s   Wilson, C D ^a   Israel, F P ^b   Serjeant, S ^c   Bendo, G J ^d   Brinks, E ^e   Clements, D L ^d   Irwin, J A ^f   Knapen, J H ^g   Leech, J ^h   Matthews, H E ⁱ   Muhle S ^j   Mortimer, A M J ^k   Petitpas, G ^l   Sinukoff, E ^a   Spekkens, K ^m   Tan, B K ^h   Tilanus, R P J ^n,o   Usero, A ^p   Van Der Werf, P P ^b   Vlahakis, C ^b   Wiegert, T ^q   Zhu, M ^r   more..

^a MCMASTER UNIVERSITY   (Canada)

^b LEIDEN UNIVERSITY   (Netherlands)

^c OPEN UNIVERSITY   (United Kingdom)

^d IMPERIAL COLLEGE LONDON   (United Kingdom)

^e UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^f QUEEN S UNIVERSITY   (Canada)

^g INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^h UNIVERSITY OF OXFORD   (United Kingdom)

ⁱ NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^j JOINT INSTITUTE FOR VLBI IN EUROPE   (Netherlands)

^k UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^l HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^m ROYAL MILITARY COLLEGE OF CANADA   (Canada)

ⁿ UNIVERSITY OF HAWAII   (United States)

^o Netherlands Organization for Scientific Research   (Netherlands)

^p OBSERVATORIO ASTRONÓMICO NACIONAL   (Spain)

^q UNIVERSITY OF MANITOBA   (Canada)

^r CHINESE ACADEMY OF SCIENCES   (China)

^s UNIVERSITY OF WESTERN AUSTRALIA   (Australia)

more..

Author keywords

Galaxies: individual (NGC 628, NGC 3521, NGC 3627); Galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: spiral; Galaxies: star formation; ISM: molecules

Indexed keywords

EID: 77951105282     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/714/1/571     Document Type: Article

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