The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission fro...
The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83
About this item
Full title
Author / Creator
Jones, A G , Bendo, G J , Baes, M , Boquien, M , Boselli, A , De Looze, I , Fritz, J , Galliano, F , Hughes, T M , Lebouteiller, V , N Lu , Madden, S C , Remy-Ruyer, A , Smith, M W L , Spinoglio, L and Zijlstra, A A
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
We examine the relation between polycyclic aromatic hydrocarbon (PAH) emission at 8 microns and far-infrared emission from hot dust grains at 24 microns and from large dust grains at 160 and 250 microns in the nearby spiral galaxies NGC 2403 and M83 using data from the Spitzer Space Telescope and Herschel Space Observatory. We find that the PAH emi...
Alternative Titles
Full title
The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83
Authors, Artists and Contributors
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2083091853
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2083091853
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1412.7344
