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The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83
A. G. Jones, G. J. Bendo, M. Baes +13
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…
Insights into gas heating and cooling in the disc of NGC 891 from Herschel far-infrared spectroscopy
T. M. Hughes, K. Foyle, M. R. P. Schirm +15
We present Herschel PACS and SPIRE spectroscopy of the most important far-infrared cooling lines in the nearby edge-on spiral galaxy, NGC 891: [CII] 158 m, [NII] 122, 205 m,…
A Spitzer Space Telescope survey of extreme Asymptotic Giant Branch stars in M32
O. C. Jones, I. McDonald, R. M. Rich +4
We investigate the population of cool, evolved stars in the Local Group dwarf elliptical galaxy M32, using Infrared Array Camera observations from the Spitzer Space Telescope. We c…
Quantifying the Heating Sources for Mid-infrared Dust Emissions in Galaxies: The Case of M 81
Nanyao Lu, G. J. Bendo, A. Boselli +12
With the newly available SPIRE images at 250 and 500 micron from Herschel Space Observatory, we study quantitative correlations over a sub-kpc scale among three distinct emission c…
The Herschel Virgo Cluster Survey. XVII. SPIRE point-source catalogs and number counts
Ciro Pappalardo, George J. Bendo, Simone Bianchi +19
We present three independent catalogs of point-sources extracted from SPIRE images at 250, 350, and 500 micron as a part of the Herschel Virgo Cluster Survey (HeViCS). The source p…
High-resolution, 3D radiative transfer modeling : I. The grand-design spiral galaxy M51
Ilse De Looze, Jacopo Fritz, Maarten Baes +20
Context: Dust reprocesses about half of the stellar radiation in galaxies. The thermal re-emission by dust of absorbed energy is considered driven merely by young stars and, conseq…