Physical conditions in the ionized gas of 30 doradus

Astrophysical Journal

Volumn 694, Issue 1, 2009, Pages 84-106

  Indebetouw, R ^a,b   De Messieres G E ^a   Madden, S ^c   Engelbracht, C ^d   Smith, J D ^e   Meixner, M ^f   Brandl, B ^g   Smith, L J ^f,h   Boulanger, F ⁱ   Galliano, F ^j   Gordon, K ^d   Hora, J L ^k   Sewilo, M ^f   Tielens, A G G M ^l   Werner, M ^m   Wolfire, M G ^j  

^a UNIVERSITY OF VIRGINIA   (United States)

^b NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d UNIVERSITY OF ARIZONA   (United States)

^e UNIVERSITY OF TOLEDO   (United States)

^f AURA for the European Space Agency   (United States)

^g LEIDEN UNIVERSITY   (Netherlands)

^h UNIVERSITY COLLEGE LONDON   (United Kingdom)

ⁱ CNRS   (France)

^j UNIVERSITY OF MARYLAND   (United States)

^k HARVARD UNIVERSITY   (United States)

^l NASA AMES RESEARCH CENTER   (United States)

^m CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

H ii regions; Infrared: ISM; ISM: individual (30 Doradus); Magellanic Clouds

Indexed keywords

EID: 75149149200     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/694/1/84     Document Type: Article

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