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Some Results from the Herschel Virgo Cluster Survey (HeViCS)

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If you have a question about this talk, please contact David Titterington.

The Herschel Virgo Cluster Survey (HeViCS) covered a continuous area of 60 square degrees of the Virgo cluster in 286 hours of Herschel observing time. Making use of both PACS and Spire maps of almost the whole cluster, maps have been made at wavelengths from 100-500 micron. This survey provides a blind survey of the dust in galaxies in the cluster environment (free of the effects of selection at other wavelengths). I will give a summary of the main results obtained so far relating to 1) dust inside galaxies, 2) dust outside galaxies, and 3) dust survival times.

This talk is part of the Cavendish Astrophysics Seminars series.

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