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The Identification of Dust Heating Mechanisms in Nearby Galaxies Using Herschel 160/250 and 250/350 Mu M Surface Brightness Ratios

AuthID
P-00G-278

Author(s)

Bendo, GJ

Baes, M

Bianchi, S

Boquien, M

Boselli, A

Cooray, A

Cortese, L

De Looze, I

Alighieri, SD

Fritz, J

Gentile, G

Hughes, TM

Lu, N

Pappalardo, C

Smith, MWL

Spinoglio, L

Viaene, S

Vlahakis, C

Tipo de Documento

Article

Year published

2015

Publicado

in MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN: 0035-8711

Volume: 448, Número: 1, Páginas: 135-167 (33)

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Publication Identifiers

DOI: 10.1093/mnras/stu1841

SCOPUS: 2-s2.0-85015629555

Wos: WOS:000350273500011

Source Identifiers

ISSN: 0035-8711

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The Identification of Dust Heating Mechanisms in Nearby Galaxies Using Herschel 160/250 and 250/350 Mu M Surface Brightness Ratios

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The Identification of Dust Heating Mechanisms in Nearby Galaxies Using Herschel 160/250 and 250/350 Mu M Surface Brightness Ratios

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