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The Herschel Virgo Cluster Survey XII: FIR properties of optically-selected Virgo Cluster galaxies
R. Auld, S. Bianchi, M. W. L. Smith +24
The Herschel Virgo Cluster Survey (HeViCS) is the deepest, confusion-limited survey of the Virgo Cluster at far-infrared (FIR) wavelengths. The entire survey at full depth covers $…
The dust energy balance in the edge-on spiral galaxy NGC 4565
Ilse De Looze, Maarten Baes, George J. Bendo +20
We combine new dust continuum observations of the edge-on spiral galaxy NGC 4565 in all Herschel/SPIRE (250, 350, 500 micron) wavebands, obtained as part of the Herschel Reference…
Submillimetre Photometry of 323 Nearby Galaxies from the Herschel Reference Survey
L. Ciesla, A. Boselli, M. W. L. Smith +23
The Herschel Reference Survey (HRS) is a guaranteed time Herschel key project aimed at studying the physical properties of the interstellar medium in galaxies of the nearby univers…
The Herschel Virgo Cluster Survey: X.The relationship between cold dust and molecular gas content in Virgo spirals
Edvige Corbelli, Simone Bianchi, Luca Cortese +16
Using the far-infrared emission, as observed by the Herschel Virgo Cluster Survey (HeViCS), and the integrated HI and CO brightness, we infer the dust and total gas mass for a magn…
Herschel and JCMT observations of the early-type dwarf galaxy NGC 205
I. De Looze, M. Baes, T. J. Parkin +18
We present Herschel dust continuum, James Clerk Maxwell Telescope CO(3-2) observations and a search for [CII] 158 micron and [OI] 63 micron spectral line emission for the brightest…
Can dust emission be used to map the interstellar medium in high-redshift galaxies? Results from the Herschel Reference Survey
Stephen Eales, Matthew W. L. Smith, Robbie Auld +23
It has often been suggested that an alternative to the standard CO/21-cm method for estimating the mass of the interstellar medium (ISM) in a galaxy might be to estimate the mass o…