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

G.J J Bendo, M. Baes, S. Bianchi, A. Boquien, A. Boselli, A. Cooray, Luca Cortese, I. De Looze, S. di Serego Alighieri, J. Fritz, G. Gentile, T.M. M. Hughes, N. Lu, C Pappalardo, M.W.L W.L Smith, L. Spinoglio, S. Viaene, C. Vlahakis

Research output: Contribution to journalArticle

40 Citations (Scopus)
Original languageEnglish
Pages (from-to)135-167
Number of pages33
JournalMonthly Notices of the Royal Astronomical Society
Volume448
Issue number1
DOIs
Publication statusPublished - 2015
Externally publishedYes

Cite this

Bendo, G. J. J., Baes, M., Bianchi, S., Boquien, A., Boselli, A., Cooray, A., Cortese, L., De Looze, I., di Serego Alighieri, S., Fritz, J., Gentile, G., Hughes, T. M. M., Lu, N., Pappalardo, C., Smith, M. W. L. W. L., Spinoglio, L., Viaene, S., & Vlahakis, C. (2015). The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350μm surface brightness ratios. Monthly Notices of the Royal Astronomical Society, 448(1), 135-167. https://doi.org/10.1093/mnras/stu1841