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

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, L. Spinoglio, S. Viaene, C. Vlahakis

    Research output: Contribution to journalArticlepeer-review

    Fingerprint

    Dive into the research topics of 'The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios'. Together they form a unique fingerprint.

    Physics