A detailed study of the radio-FIR correlation in NGC6946 with Herschel -PACS/SPIRE from KINGFISH

Astronomy and Astrophysics

Volumn 552, Issue , 2013, Pages

  Tabatabaei, F S ^a   Schinnerer, E ^a   Murphy, E J ^b   Beck, R ^c   Groves, B ^a   Meidt, S ^a   Krause, M ^c   Rix, H W ^a   Sandstrom, K ^a   Crocker, A F ^d   Galametz, M ^e   Helou, G ^f   Wilson, C D ^g   Kennicutt, R ^e   Calzetti, D ^d   Draine, B ^h   Aniano, G ^h   Dale, D ⁱ   Dumas, G ^j   Engelbracht, C W ^k,l   Gordon, K D ^m   Hinz, J ^k   Kreckel, K ^a   Montiel, E ^k   Roussel, H ⁿ   more..

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b CARNEGIE OBSERVATORIES   (United States)

^c MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^d UNIVERSITY OF MASSACHUSETTS   (United States)

^e UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g MCMASTER UNIVERSITY   (Canada)

^h PRINCETON UNIVERSITY OBSERVATORY   (United States)

ⁱ UNIVERSITY OF WYOMING   (United States)

^j IRAM   (France)

^k UNIVERSITY OF ARIZONA   (United States)

^l RAYTHEON COMPANY   (United States)

^m STScI   (United States)

ⁿ INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

more..

Author keywords

galaxies: individual: NGC6946; galaxies: star formation; infrared: ISM; ISM: magnetic fields; radio continuum: ISM

Indexed keywords

GALAXIES: INDIVIDUALS; GALAXIES: STAR FORMATION; INFRARED: ISM; ISM: MAGNETIC FIELDS; RADIO CONTINUUM: ISM;

DENSITY OF GASES; DIFFUSION; DUST; ENERGY DISSIPATION; MAGNETIC FIELDS; STARS; SYNCHROTRON RADIATION;

GALAXIES;

EID: 84875158369     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220249     Document Type: Article

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