87 citations · 332 across the 6 of their papers we have counts for
6 papers
Can planet formation resolve the dust budget crisis in high redshift galaxies?
D. H. Forgan, K. Rowlands, H. L. Gomez +4
The process of planet formation offers a rich source of dust production via grain growth in protostellar discs, and via grinding of larger bodies in debris disc systems. Chemical e…
Using dust, gas and stellar mass selected samples to probe dust sources and sinks in low metallicity galaxies
P. De Vis, H. L. Gomez, S. P. Schofield +8
We combine samples of nearby galaxies with Herschel photometry selected on their dust, metal, HI, and stellar mass content, and compare these to chemical evolution models in order…
The Galaxy End Sequence
Stephen Eales, Pieter de Vis, Matthew Smith +4
A common assumption is that galaxies fall in two distinct regions on a plot of specific star-formation rate (SSFR) versus galaxy stellar mass: a star-forming Galaxy Main Sequence (…
Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations
P. De Vis, L. Dunne, S. Maddox +19
We present a study of the dust, stars and atomic gas (HI) in an HI-selected sample of local galaxies (z<0.035) in the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) f…
An Empirical Determination of the Dust Mass Absorption Coefficient, , Using the Herschel Reference Survey
Christopher J. R. Clark, Simon P. Schofield, Haley L. Gomez +1
We use the published photometry and spectroscopy of 22 galaxies in the Herschel Reference Survey to determine that the value of the dust mass absorption coefficient at a wa…
Herschel-ATLAS: The Surprising Diversity of Dust-Selected Galaxies in the Local Submillimetre Universe
Christopher J. R. Clark, Loretta Dunne, Haley L. Gomez +19
We present the properties of the first 250 m blind sample of nearby galaxies (15 < D < 46 Mpc) containing 42 objects from the Herschel Astrophysical Terahertz Large Area Survey…