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Quantifying the Heating Sources for Mid-infrared...
Preprint

Quantifying the Heating Sources for Mid-infrared Dust Emissions in Galaxies: The Case of M 81

Abstract

With the newly available SPIRE images at 250 and 500 micron from Herschel Space Observatory, we study quantitative correlations over a sub-kpc scale

Authors

Lu N; Bendo GJ; Boselli A; Baes M; Wu. H; Madden SC; De Looze I; Rémy-Ruyer A; Boquien M; Wilson CD

Publication date

October 14, 2014

DOI

10.48550/arxiv.1410.3874

Preprint server

arXiv