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Extreme Feedback and the Epoch of Reionization: Clues in the Local Universe

Heckman, Timothy M. and Borthakuri, Sanchayeeta and Overzier, Roderik and Kauffmann, Guinevere and Basu-Zych, Antara and Leitherer, Claus and Sembach, Ken and Martin, D. Chris and Rich, R. Michael and Schiminovich, David and Seibert, Mark (2011) Extreme Feedback and the Epoch of Reionization: Clues in the Local Universe. Astrophysical Journal, 730 (1). Art. No. 5. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20110414-085411947

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Abstract

The source responsible for reionizing the universe at z > 6 remains uncertain. While an energetically adequate population of star-forming galaxies may be in place, it is unknown whether a large enough fraction of their ionizing radiation can escape into the intergalactic medium. Attempts to measure this escape fraction in intensely star-forming galaxies at lower redshifts have largely yielded upper limits. In this paper, we present new Hubble Space Telescope Cosmic Origins Spectrograph and archival Far-Ultraviolet Spectroscopic Explorer (FUSE) far-UV spectroscopy of a sample of 11 Lyman Break Analogs (LBAs), a rare population of local galaxies that strongly resemble the high-z Lyman Break galaxies. We combine these data with Sloan Digital Sky Survey optical spectra and Spitzer photometry. We also analyze archival FUSE observations of 15 typical UV-bright local starbursts. We find evidence of small covering factors for optically thick neutral gas in three cases. This is based on two independent pieces of evidence: a significant residual intensity in the cores of the strongest interstellar absorption-lines tracing neutral gas and a small ratio of extinction-corrected Hα to UV plus far-IR luminosities. These objects represent three of the four LBAs that contain a young, very compact (~10^2 pc), and highly massive (~10^9 M_⊙) dominant central object (DCO). These three objects also differ from the other galaxies in showing a significant amount of blueshifted Lyα emission, which may be related to the low covering factor of neutral gas. All four LBAs with DCOs in our sample show extremely high velocity outflows of interstellar gas, with line centroids blueshifted by about 700 km s^(–1) and maximum outflow velocities reaching at least 1500 km s^(–1). We show that these properties are consistent with an outflow driven by a powerful starburst that is exceptionally compact. We speculate that such extreme feedback may be required to enable the escape of ionizing radiation from star-forming galaxies.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/730/1/5DOIArticle
http://iopscience.iop.org/0004-637X/730/1/5PublisherArticle
Additional Information:© 2011 American Astronomical Society. Received 2010 November 17; accepted 2011 January 19; published 2011 February 23. Based on observations with the NASA/ESA Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. The observations are associated with GO programs 10920, 11107, and 11727. Facilities: HST(COS), GALEX, Spitzer
Group:Space Astrophysics Laboratory
Funders:
Funding AgencyGrant Number
NASANAS 5-26555
Subject Keywords:galaxies: evolution; galaxies: high-redshift; galaxies: ISM; galaxies: kinematics and dynamics; intergalactic medium
Classification Code:PACS: 98.62.Ai; 98.54.Ep; 98.62.Py; 95.30.Ky; 98.62.Dm; 98.62.Ra
Record Number:CaltechAUTHORS:20110414-085411947
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20110414-085411947
Official Citation:Extreme Feedback and the Epoch of Reionization: Clues in the Local Universe Timothy M. Heckman, Sanchayeeta Borthakur, Roderik Overzier, Guinevere Kauffmann, Antara Basu-Zych, Claus Leitherer, Ken Sembach, D. Chris Martin, R. Michael Rich, David Schiminovich and Mark Seibert doi: 10.1088/0004-637X/730/1/5
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:23324
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:15 Apr 2011 16:00
Last Modified:28 Aug 2016 20:31

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