100 μ m and 160 μ m emission as resolved star-formation rate estimators in M 33 (HERM33ES)

Astronomy and Astrophysics

Volumn 518, Issue 8, 2010, Pages

  Boquien, M ^a   Calzetti, D ^a   Kramer, C ^b   Xilouris, E M ^c   Bertoldi, F ^d   Braine, J ^e   Buchbender, C ^b   Combes, F ^f   Israel, F ^g   Koribalski, B ^h   Lord, S ⁱ   Quintana Lacaci, G ^b   Relano M ^j   Rollig M ^k   Stacey, G ^l   Tabatabaei, F S ^m   Tilanus, R P J ⁿ   Van Der Tak, F ^o   Van Der Werf, P ^g   Verley, S ^p  

^a UNIVERSITY OF MASSACHUSETTS   (United States)

^b Institute de Radioastronomie Millimétrique IRAM Núcleo Central   (Spain)

^c NATIONAL OBSERVATORY OF ATHENS   (Greece)

^d UNIVERSITY OF BONN   (Germany)

^e LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

^f OBSERVATOIRE DE PARIS   (France)

^g LEIDEN UNIVERSITY   (Netherlands)

^h CSIRO   (Australia)

ⁱ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^j UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^k UNIVERSITY OF COLOGNE   (Germany)

^l Department of Obstetrics Gynecology   (United States)

^m MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

ⁿ JAC   (United States)

^o SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^p UNIVERSITY OF GRANADA   (Spain)

more..

Author keywords

Galaxies: individual: M 33; Galaxies: spiral; Galaxies: star formation; Infrared: galaxies

Indexed keywords

DUST; ESTIMATION;

DIFFUSE EMISSION; DYNAMIC RANGE; FORMATION RATES; GALAXIES: INDIVIDUAL: M33; GALAXIES: SPIRAL; GALAXIES: STAR FORMATION; H II REGIONS; INFRARED BANDS; INFRARED LUMINOSITY; INFRARED: GALAXIES; LINEAR ESTIMATORS; STAR FORMATIONS; STAR-FORMING REGION; SUPERLINEAR;

GALAXIES;

EID: 77957850626     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014649     Document Type: Article

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