Alexander, D.M., Simpson, J.M., Harrison, C.M. et al. (14 more authors) (2016) ALMA observations of a $z$ ≈ 3.1 Protocluster: Star Formation from Active Galactic Nuclei and Lyman-Alpha Blobs in an Overdense Environment. Monthly Notices of the Royal Astronomical Society, 461 (3). pp. 2944-2952. ISSN 0035-8711
Abstract
We exploit ALMA 870 µm observations to measure the star-formation rates (SFRs) of eight X-ray detected Active Galactic Nuclei (AGNs) in a z ≈ 3.1 protocluster, four of which reside in extended Ly α haloes (often termed Ly α blobs: LABs). Three of the AGNs are detected by ALMA and have implied SFRs of ≈ 220–410 M⊙ yr−1 ; the non detection of the other five AGNs places SFR upper limits of <∼ 210 M⊙ yr−1 . The mean SFR of the protocluster AGNs (≈ 110–210 M⊙ yr−1 ) is consistent (within a factor of ≈ 0.7–2.3) with that found for co-eval AGNs in the field, implying that the galaxy growth is not significantly accelerated in these systems. However, when also considering ALMA data from the literature, we find evidence for elevated mean SFRs (up-to a factor of ≈ 5.9 over the field) for AGNs at the protocluster core, indicating that galaxy growth is significantly accelerated in the central regions of the protocluster. We also show that all of the four protocluster LABs are associated with an ALMA counterpart within the extent of their Ly α emission. The SFRs of the ALMA sources within the LABs (≈ 150–410 M⊙ yr−1 ) are consistent with those expected for co-eval massive star-forming galaxies in the field. Furthermore, the two giant LABs (with physical extents of >∼ 100 kpc) do not host more luminous star formation than the smaller LABs, despite being an order of magnitude brighter in Ly α emission. We use these results to discuss star formation as the power source of LABs.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2016 Oxford University Press. This is an author produced version of a paper subsequently published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy. |
Keywords: | galaxies: evolution; galaxies: star formation; galaxies: active; quasars: general; submillimetre: galaxies |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield) |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 21 Nov 2016 16:34 |
Last Modified: | 24 Mar 2018 14:45 |
Published Version: | http://doi.org/10.1093/mnras/stw1509 |
Status: | Published |
Publisher: | Oxford University Press |
Refereed: | Yes |
Identification Number: | 10.1093/mnras/stw1509 |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:107849 |