A Herschel and CARMA view of CO and [C II] in Hickson Compact groups
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1.
Infrared Processing and Analysis Center
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2.
University of Granada
Abstract
Understanding the evolution of galaxies from the starforming blue cloud to the quiescent red sequence has been revolutionized by observations taken with Herschel Space Observatory, and the onset of the era of sensitive millimeter interferometers, allowing astronomers to probe both cold dust as well as the cool interstellar medium in a large set of galaxies with unprecedented sensitivity. Recent Herschel observations of of H_2-bright Hickson Compact Groups of galaxies (HCGs) has shown that [CII] may be boosted in diffuse shocked gas. CARMA CO(1-0) observations of these [CII]-bright HCGs has shown that these turbulent systems also can show suppression of SF. Here we present preliminary results from observations of HCGs with Herschel and CARMA, and their [CII] and CO(1-0) properties to discuss how shocks influence galaxy transitions and star formation.
Additional Information
© 2015 International Astronomical Union. Proceedings IAU Symposium No. 309. Published online: 09 February 2015. K.A. is supported by funding through Herschel, a European Space Agency Cornerstone Mission with significant participation by NASA, through an award issued by JPL/Caltech. U.L. acknowledges support by the research projects AYA2011-24728 from the Spanish Ministerio de Ciencia y Educación and the Junta de Andalucía (Spain) grants FQM108. Support for CARMA construction was derived from the Gordon and Betty Moore Foundation, the Kenneth T. and Eileen L. Norris Foundation, the James S. McDonnell Foundation, the Associates of the California Institute of Technology, the University of Chicago, the states of California, Illinois, and Maryland, and the National Science Foundation. Ongoing CARMA development and operations are supported by the National Science Foundation under a cooperative agreement, and by the CARMA partner universities. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. This work is based [in part] on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA.Attached Files
Published - S1743921314009624a.pdf
Submitted - 1409.6063.pdf
Files
1409.6063.pdf
Additional details
Identifiers
- Eprint ID
- 50199
- Resolver ID
- CaltechAUTHORS:20141006-084345527
Related works
- Describes
- http://arxiv.org/abs/1409.6063 (URL)
- https://galaxy3d.univie.ac.at/ (URL)
Funding
- European Space Agency (ESA)
- NASA/JPL/Caltech
- Ministerio de Ciencia y Educaciόn (MEC)
- AYA2011-24728
- Junta de Andalucía
- FQM108
- Gordon and Betty Moore Foundation
- Kenneth T. and Eileen L. Norris Foundation
- James S. McDonnell Foundation
- Caltech Associates
- University of Chicago
- State of California
- State of Illinois
- State of Maryland
- NSF
Dates
- Created
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2014-10-09Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field