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Resolving the Galaxies within a Giant Lyα Nebula: Witnessing the Formation of a Galaxy Group?

Prescott, Moire K. M. and Dey, Arjun and Brodwin, Mark and Chaffee, Frederic H. and Desai, Vandana and Eisenhardt, Peter and Le Floc'h, Emeric and Jannuzi, Buell T. and Kashikawa, Nobunari and Matsuda, Yuichi and Soifer, B. T. (2012) Resolving the Galaxies within a Giant Lyα Nebula: Witnessing the Formation of a Galaxy Group? Astrophysical Journal, 752 (2). Art. No. 86. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20120723-130359266

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Abstract

Detailed analysis of the substructure of Lyα nebulae can put important constraints on the physical mechanisms at work and the properties of galaxies forming within them. Using high-resolution Hubble Space Telescope (HST) imaging of a Lyα nebula at z ≈ 2.656, we have taken a census of the compact galaxies in the vicinity, used optical/near-infrared colors to select system members, and put constraints on the morphology of the spatially extended emission. The system is characterized by (1) a population of compact, low-luminosity (~0.1 L*) sources—17 primarily young, small (R_e ≈ 1-2 kpc), disky galaxies including an obscured active galactic nucleus—that are all substantially offset (≳20 kpc) from the line-emitting nebula; (2) the lack of a central galaxy at or near the peak of the Lyα emission; and (3) several nearly coincident, spatially extended emission components—Lyα, He II, and UV continuum—that are extremely smooth. These morphological findings are difficult to reconcile with theoretical models that invoke outflows, cold flows, or resonant scattering, suggesting that while all of these physical phenomena may be occurring, they are not sufficient to explain the powering and large extent of Lyα nebulae. In addition, although the compact galaxies within the system are irrelevant as power sources, the region is significantly overdense relative to the field galaxy population (by at least a factor of four). These observations provide the first estimate of the luminosity function of galaxies within an individual Lyα nebula system and suggest that large Lyα nebulae may be the seeds of galaxy groups or low-mass clusters.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/752/2/86DOIArticle
http://iopscience.iop.org/0004-637X/752/2/86PublisherArticle
ORCID:
AuthorORCID
Dey, Arjun0000-0002-4928-4003
Brodwin, Mark0000-0002-4208-798X
Desai, Vandana0000-0002-1340-0543
Additional Information:© 2012 American Astronomical Society. Received 2011 May 25; accepted 2012 April 11; published 2012 May 30. The authors thank Kate Brand, Galina Soutchkova, and SangeetaMalhotra for their assistance with the HST observation planning and execution. We are grateful to Crystal Martin, Kristian Finlator, Avi Loeb, Dan Weedman, Tommaso Treu, Matt Auger, and the anonymous referee for useful discussions and suggestions. M.K.M.P. acknowledges support from an NSF Graduate Research Fellowship, a P.E.O. Fellowship, and a TABASGO Prize Postdoctoral Fellowship. This work was based on observations made with the NASA/ESA Hubble Space Telescope (HST Cycle 14; GO#10591), obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. This work is also based in part on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan, and on data from the NOAO Deep Wide-Field Survey (B. Jannuzi, A. Dey) as distributed by the NOAO Science Archive. A.D. and B.T.J.’s research activities are supported by NOAO. NOAO is operated by the Association of Universities for Research in Astronomy (AURA), Inc. under a cooperative agreement with the National Science Foundation. V.D. and B.T.S. are supported by the Spitzer Space Telescope project, which is managed by JPL on behalf of NASA. Facilities: HST, Subaru, Mayall
Funders:
Funding AgencyGrant Number
NSF Graduate Research FellowshipUNSPECIFIED
TABASGO Prize Postdoctoral FellowshipUNSPECIFIED
National Optical Astronomy Observatory (NOAO)UNSPECIFIED
Spitzer Space TelescopeUNSPECIFIED
P.E.O. FellowshipUNSPECIFIED
Subject Keywords:galaxies: evolution; galaxies: formation; galaxies: high-redshift
Issue or Number:2
Record Number:CaltechAUTHORS:20120723-130359266
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20120723-130359266
Official Citation:Resolving the Galaxies within a Giant Lyα Nebula: Witnessing the Formation of a Galaxy Group? Moire K. M. Prescott et al. 2012 ApJ 752 86
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:32650
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:23 Jul 2012 23:08
Last Modified:24 Jul 2019 23:48

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