Understanding radio-selected thermal sources in M33: Ultraviolet, optical, near-infrared, Spitzer mid-infrared, and radio observations

Astrophysical Journal, Supplement Series

Volumn 162, Issue 2, 2006, Pages 329-345

  Buckalew, Brent A ^a,b   Kobulnicky, Henry A ^a   Darnel, Jonathan M ^a   Polomski, Elisha ^c   Gehrz, Robert D ^c   Humphreys, Roberta M ^c   Woodward, Charles E ^c   Hinz, Joannah L ^d   Engelbracht, C W ^d   Gordon, Karl D ^d   Misselt, K ^d   Perez Gonzalez P G ^d   Rieke, George H ^d   Willner, S P ^e   Ashby, M L ^e   Barmby, P ^e   Pahre, M A ^e   Roellig, T L ^f   Devereux, Nick ^g   Loon, Jacco Th ^h   Brandl, B ⁱ   more..

^a UNIVERSITY OF WYOMING   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c University of Minnesota   (United States)

^d UNIVERSITY OF ARIZONA   (United States)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f NASA AMES RESEARCH CENTER   (United States)

^g EMBRY RIDDLE AERONAUTICAL UNIVERSITY   (United States)

^h KEELE UNIVERSITY   (United Kingdom)

ⁱ LEIDEN UNIVERSITY   (Netherlands)

Author keywords

Dust, extinction; Galaxies: individual (M33); Galaxies: star clusters; Infrared: ISM; ISM: structure

Indexed keywords

EID: 33644923784     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/498572     Document Type: Article

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