The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios

We examined variations in the 160/250 and 250/350 μm surface brightness ratios within 24 nearby (

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Bibliographic Details
Published in:	Monthly notices of the Royal Astronomical Society 2015-03, Vol.448 (1), p.135-167
Main Authors:	Bendo, G. J., Baes, M., Bianchi, S., Boquien, M., Boselli, A., Cooray, A., Cortese, L., De Looze, I., di Serego Alighieri, S., Fritz, J., Gentile, G., Hughes, T. M., Lu, N., Pappalardo, C., Smith, M. W. L., Spinoglio, L., Viaene, S., Vlahakis, C.
Format:	Article
Language:	English
Subjects:	Astronomical models Astrophysics Dust Emission Emission analysis Galaxies Heating Physics Star formation Stellar populations Surface brightness
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