A Complete 1.1mm Survey of Perseus with Bolocam

Details A Complete 1.1mm Survey of Perseus with Bolocam A Complete 1.1mm Survey of Perseus with Bolocam

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..357..137e&link_type=abstract

The Spitzer Space Telescope: New Views of the Cosmos ASP Conference Series, Volume 357, proceedings of the conference held 9-12

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Scientific paper

We have completed a 7.5 square degree λ=1.1mm map of Perseus using Bolocam. Our map is the largest unbiased survey of Perseus at millimeter wavelengths to date, and covers the same area as the c2d Spitzer IRAC and MIPS maps of Perseus. We find that that the mass function shape is similar to that seen in other clouds and to the local IMF. Despite the large area surveyed, few new sources are found outside the known cluster regions.

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