Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 1(448), p. 135-167, 2015
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The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios
Journal article published in 2015 by
G. J. Bendo,
M. Baes 
,
S. Bianchi ,
M. Boquien,
A. Boselli,
A. Cooray,
L. Cortese,
I. De Looze,
S. di Serego Alighieri ,
J. Fritz ,
G. Gentile,
T. M. Hughes,
N. Lu,
C. Pappalardo,
M. W. L. Smith
and other authors.
,
S. Bianchi ,
M. Boquien,
A. Boselli,
A. Cooray,
L. Cortese,
I. De Looze,
S. di Serego Alighieri ,
J. Fritz ,
G. Gentile,
T. M. Hughes,
N. Lu,
C. Pappalardo,
M. W. L. Smith
and other authors.
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
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