Alatalo, Katherine and Appleton, Philip N. and Lisenfeld, Ute (2014) A Herschel and CARMA view of CO and [C II] in Hickson Compact groups. Proceedings of the International Astronomical Union, 10 . pp. 178-181. ISSN 1743-9213. doi:10.1017/S1743921314009624. https://resolver.caltech.edu/CaltechAUTHORS:20141006-084345527
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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.
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| 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. | ||||||||||||||||||||||||||||
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| Subject Keywords: | galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: formation | ||||||||||||||||||||||||||||
| DOI: | 10.1017/S1743921314009624 | ||||||||||||||||||||||||||||
| Record Number: | CaltechAUTHORS:20141006-084345527 | ||||||||||||||||||||||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20141006-084345527 | ||||||||||||||||||||||||||||
| Official Citation: | Katherine Alatalo, Philip N. Appleton and Ute Lisenfeld (2014). A Herschel and CARMA view of CO and [C ii] in Hickson Compact groups. Proceedings of the International Astronomical Union, 10, pp 178-181. doi:10.1017/S1743921314009624. | ||||||||||||||||||||||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||||||||||||||||||
| ID Code: | 50199 | ||||||||||||||||||||||||||||
| Collection: | CaltechAUTHORS | ||||||||||||||||||||||||||||
| Deposited By: | Tony Diaz | ||||||||||||||||||||||||||||
| Deposited On: | 09 Oct 2014 22:06 | ||||||||||||||||||||||||||||
| Last Modified: | 10 Nov 2021 18:53 |
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