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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,…
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…
The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 micron surface brightness ratios
G. J. Bendo, M. Baes, S. Bianchi +15
We examined variations in the 160/250 and 250/350 micron surface brightness ratios within 24 nearby (<30 Mpc) face-on spiral galaxies observed with the Herschel Space Observatory t…
The Herschel Fornax Cluster Survey II: FIR properties of optically-selected Fornax cluster galaxies
C. Fuller, J. I. Davies, R. Auld +13
The Fornax Cluster Survey (HeFoCS) is a deep, far-infrared (FIR) survey of the Fornax cluster. The survey is in 5 bands (100 - 500 m) and covers an area of…