Published 2006
| Published
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A complete 1.1mm survey of Perseus with Bolocam
Abstract
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.
Additional Information
© 2006 Astronomical Society of the Pacific. Support for this work, part of the Spitzer Legacy Science Program, was provided by NASA through contracts 1224608 and 1230782 issued by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407.Attached Files
Published - Enoch2006p9025Spitzer_Space_Telescope_New_Views_Of_The_Cosmos.pdf
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Enoch2006p9025Spitzer_Space_Telescope_New_Views_Of_The_Cosmos.pdf
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Additional details
- Eprint ID
- 22662
- Resolver ID
- CaltechAUTHORS:20110304-110358706
- 1224608
- NASA
- 1230782
- NASA
- 1407
- NASA
- NASA/JPL/Caltech
- Created
-
2011-03-04Created from EPrint's datestamp field
- Updated
-
2019-12-09Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)
- Series Name
- ASP Conference Series
- Series Volume or Issue Number
- 357