Filamentary Large-scale Structure Traced by Six Lyα Blobs at z = 2.3
Abstract
Extended nebulae of Lyα emission ("Lyα blobs") are known to be associated with overdense regions at high redshift. Here we present six large Lyα blobs in a previously known protocluster with galaxy overdensity δ ~ 7 at z = 2.3; this is the richest field of giant Lyα blobs detected to date. The blobs have linear sizes of ≳ 100 kpc and Lyα luminosities of ~10^(43) erg s^(–1). The positions of the blobs define two linear filaments with an extent of at least 12 comoving Mpc; these filaments intersect at the center of one of the blobs. Measurement of the position angles of the blobs indicates that five of the six are aligned with these filaments to within ~10°, suggesting a connection between the physical processes powering extended Lyα emission and those driving structure on larger scales.
Additional Information
© 2011 American Astronomical Society. Received 2011 August 17; accepted 2011 September 9; published 2011 September 22. Alice Shapley, Naveen Reddy, and Max Pettini provided essential contributions to the survey on which this work is based. We also thank the staffs of Palomar and Keck Observatories for assistance with the observations, Yuichi Matsuda for useful suggestions, and the referee for helpful comments. D.K.E. acknowledges support from the University of Wisconsin Research Growth Initiative, and C.C.S. from the US National Science Foundation through grants AST-0606912 and AST-0908805, with additional support from the John D. and Catherine T. MacArthur Foundation and the Peter and Patricia Gruber Foundation.Attached Files
Published - Erb2011p16046Astrophys_J_Lett.pdf
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Additional details
- Eprint ID
- 27225
- Resolver ID
- CaltechAUTHORS:20111014-095153900
- University of Wisconsin
- NSF
- AST-0606912
- NSF
- AST-0908805
- John D. and Catherine T. MacArthur Foundation
- Peter and Patricia Gruber Foundation
- Created
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2011-10-14Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field