Dust emission and star formation in Stephan's quintet

Astrophysical Journal

Volumn 725, Issue 1, 2010, Pages 955-984

  Natale, G ^a   Tuffs, R J ^a   Xu, C K ^b   Popescu, C C ^c   Fischera, J ^d   Lisenfeld, U ^e   Lu, N ^b   Appleton, P ^b   Dopita, M ^f   Duc, P A ^g   Gao, Y ^h   Reach, W ⁱ   Sulentic, J ^j   Yun, M ^k  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^d UNIVERSITY OF TORONTO   (Canada)

^e UNIVERSITY OF GRANADA   (Spain)

^f AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^g UNIVERSITÉ PARIS DIDEROT   (France)

^h CHINESE ACADEMY OF SCIENCES   (China)

ⁱ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^j INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^k UNIVERSITY OF MASSACHUSETTS   (United States)

more..

Author keywords

Dust; Extinction; Galaxies: groups: individual (HGC92); Galaxies: interactions; Galaxies: star formation; Infrared: general; Intergalactic medium

Indexed keywords

EID: 78650029691     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/725/1/955     Document Type: Article

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