A Herschel and CARMA view of CO and [C II] in Hickson Compact groups
arXiv:1409.6063 · doi:10.1017/S1743921314009624
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 H2-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.
arXiv comment4 pages, 3 figures, Proceedings for IAU Symposium 309, Galaxies in 3D across the Universe
References in corpus (24)
- The Global Schmidt Law in Star Forming Galaxies
- The CO-to-H2 Conversion Factor
- Far Infrared Spectroscopy of Normal Galaxies: Physical Conditions in the Interstellar Medium
- A 158 Micron [CII] Line Survey of Galaxies at z ~ 1 to 2: An Indicator of Star Formation in the Early Universe
- Where is the Neutral Atomic Gas in Hickson Groups?
- Explaining the [CII]158um Deficit in Luminous Infrared Galaxies - First Results from a Herschel/PACS Study of the GOALS Sample
- The [CII] 158 um Line Deficit in Ultraluminous Infrared Galaxies Revisited
- The ATLAS3D project - XVIII. CARMA CO imaging survey of early-type galaxies
- Compact groups of galaxies
- The reliability of [CII] as a star formation rate indicator
- Spitzer Reveals Hidden Quasar Nuclei in Some Powerful FR II Radio Galaxies
- Shock-Enhanced C+ Emission and the Detection of H2O from Stephan's Quintet's Group-Wide Shock using Herschel
- Galaxy Evolution in Hickson Compact Groups: The Role of Ram Pressure Stripping and Strangulation
- The Infrared Properties of Hickson Compact Groups
- Turbulent molecular gas and star formation in the shocked intergalactic medium of Stephan's Quintet
- Detection of Diffuse Neutral Intragroup Medium in Hickson Compact Groups
- Enhanced Warm H2 Emission in the Compact Group Mid-Infrared "Green Valley"
- Mid-Infrared Evidence for Accelerated Evolution in Compact Group Galaxies
- A mid-IR study of Hickson Compact Groups II. Multi-wavelength analysis of the complete GALEX-Spitzer Sample
- A mid-IR study of Hickson Compact Groups I : Probing the Effects of Environment in Galaxy Interactions
- Detection of Powerful Mid-IR H2 Emission in the Bridge between the Taffy Galaxies
- Strong Far-IR Cooling Lines, Peculiar CO Kinematics and Possible Star Formation Suppression in Hickson Compact Group 57
- The Optical Green Valley vs Mid-IR Canyon in Compact Groups
- Examining the Role of Environment in a Comprehensive Sample of Compact Groups