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Metal-Enriched Gaseous Halos around Distant Radio Galaxies: Clues to Feedback in Galaxy Formation

Reuland, Michiel and van Breugel, Wil and de Vries, Wim and Dopita, Michael A. and Dey, Arjun and Miley, George and Röttgering, Huub and Venemans, Bram and Stanford, S. A. and Lacy, Mark and Spinrad, Hy and Dawson, Steve and Stern, Daniel and Bunker, Andrew (2007) Metal-Enriched Gaseous Halos around Distant Radio Galaxies: Clues to Feedback in Galaxy Formation. Astronomical Journal, 133 (6). pp. 2607-2623. ISSN 0004-6256. http://resolver.caltech.edu/CaltechAUTHORS:20091109-140229178

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Abstract

We present the results of an optical and near-IR spectroscopic study of giant nebular emission-line halos associated with three z > 3 radio galaxies, 4C 41.17, 4C 60.07, and B2 0902+34. Previous deep narrowband Lyα imaging revealed complex morphologies with sizes up to 100 kpc, possibly connected to outflows and AGN feedback from the central regions. The outer regions of these halos show quiet kinematics with typical velocity dispersions of a few hundred km s^(-1) and velocity shears that can mostly be interpreted as being due to rotation. The inner regions show shocked cocoons of gas closely associated with the radio lobes. These display disturbed kinematics and have expansion velocities and/or velocity dispersions >1000 km s^(-1). The core region is chemically evolved, and we also find spectroscopic evidence for the ejection of enriched material in 4C 41.17 up to a distance of ≈60 kpc along the radio axis. The dynamical structures traced in the Lyα line are, in most cases, closely echoed in the carbon and oxygen lines. This shows that the Lyα line is produced in a highly clumped medium of small filling factor and can therefore be used as a tracer of the dynamics of high-redshift radio galaxies (HzRGs). We conclude that these HzRGs are undergoing a final jet-induced phase of star formation with ejection of most of their interstellar medium before becoming "red and dead" elliptical galaxies.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/516571DOIArticle
http://www.iop.org/EJ/abstract/1538-3881/133/6/2607/PublisherArticle
ORCID:
AuthorORCID
Stern, Daniel0000-0003-2686-9241
Additional Information:© 2007 The American Astronomical Society. Received 2006 July 24; accepted 2007 February 20. We thank all the staff at the W.M. Keck Observatory for their excellent support. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most grateful to have the opportunity to conduct observations from this mountain. M. R. thanks Mario Livio and the Space Telescope Science Institute for generous hospitality. This work was performed under the auspices of the US Department of Energy, National Nuclear Security Administration, by the University of California, Lawrence Livermore National Laboratory, under contract W-7405-Eng-48. W. v. B. acknowledges support for radio galaxy studies at the Institute for Geophysics and Planetary Physics at Lawrence Livermore National Laboratory and at UC Merced, including the work reported here, with the Hubble, Spitzer, and Chandra space telescopes via NASA grants HST GO-9779, GO-10127, SST GO-3482, SST GO- 3329, and Chandra/CXO GO-06701011. M. D. acknowledges the support of the ANU and the Australian Research Council (ARC) for his ARC Australian Federation Fellowship, as well as the ARC Discovery projects DP0208445 and DP0664434. This work was supported by the European Community Research and Training Network program, The Physics of the Intergalactic Medium. A. D.’s research is supported by NOAO, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the National Science Foundation.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)W-7405-ENG-48
NASAHST GO-9779
NASAGO-10127
NASASST GO-3482
NASASST GO-3329
NASAGO-06701011
Australian Research CouncilDP0208445
Australian Research CouncilDP0664434
Marie Curie FellowshipUNSPECIFIED
National Optical Astronomy Observatory (NOAO)UNSPECIFIED
NSFUNSPECIFIED
Subject Keywords:galaxies : active; galaxies : formation; galaxies : high-redshift; galaxies : individual (B2 0902+34, 4C 60.07, 4C 41.17); quasars : emission lines
Issue or Number:6
Record Number:CaltechAUTHORS:20091109-140229178
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20091109-140229178
Official Citation:Metal-Enriched Gaseous Halos around Distant Radio Galaxies: Clues to Feedback in Galaxy Formation Michiel Reuland, Wil van Breugel, Wim de Vries, Michael A. Dopita, Arjun Dey, George Miley, Huub Röttgering, Bram Venemans, S. A. Stanford, Mark Lacy, Hy Spinrad, Steve Dawson, Daniel Stern, and Andrew Bunker 2007 The Astronomical Journal 133 2607-2623 doi: 10.1086/516571
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:16628
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:16 Nov 2009 17:06
Last Modified:20 Oct 2017 20:11

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