MIT Libraries logoDSpace@MIT

MIT
View Item 
  • DSpace@MIT Home
  • MIT Open Access Articles
  • MIT Open Access Articles
  • View Item
  • DSpace@MIT Home
  • MIT Open Access Articles
  • MIT Open Access Articles
  • View Item
JavaScript is disabled for your browser. Some features of this site may not work without it.

A DEEP SEARCH FOR FAINT GALAXIES ASSOCIATED WITH VERY LOW REDSHIFT C iv ABSORBERS. III. THE MASS- AND ENVIRONMENT-DEPENDENT CIRCUMGALACTIC MEDIUM

Author(s)
Burchett, Joseph N.; Tripp, Todd M.; Bordoloi, Rongmon; Werk, Jessica K.; Prochaska, J. Xavier; Tumlinson, Jason; Willmer, C. N. A.; O’Meara, John; Katz, Neal; ... Show more Show less
Thumbnail
DownloadBurchett-2016-A DEEP SEARCH FOR FAINT GALAXIES.pdf (2.963Mb)
PUBLISHER_POLICY

Publisher Policy

Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.

Terms of use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Metadata
Show full item record
Abstract
Using Hubble Space Telescope Cosmic Origins Spectrograph observations of 89 QSO sightlines through the Sloan Digital Sky Survey footprint, we study the relationships between C iv absorption systems and the properties of nearby galaxies, as well as the large-scale environment. To maintain sensitivity to very faint galaxies, we restrict our sample to 0.0015 < z < 0.015, which defines a complete galaxy survey to L ≳ 0.01 L* or stellar mass M*≳ 10⁸M [subscript ⊙]. We report two principal findings. First, for galaxies with impact parameter ρ < 1r[subscript vir], C IV detection strongly depends on the luminosity/stellar mass of the nearby galaxy. C IV is preferentially associated with galaxies with M[subscript *] > 10 [superscript 9.5] M [subscript ⊙] lower-mass galaxies rarely exhibit significant C IV absorption (covering fraction f [subscript C = 9 [ subscript-6] [subscript +12] % for 11 galaxies with M[subscript *] < 10 [superscript 9.5]M [subscript ⊙]. Second, C IV detection within the M* > 10 [superscript 9.5]M [subscript ⊙] population depends on environment. Using a fixed-aperture environmental density metric for galaxies with ρ < 160 kpc at z < 0.055, we find that 57 [ subscript -13] [superscript +12]% (8/14) of galaxies in low-density regions (regions with fewer than seven L > 0.15L* galaxies within 1.5 Mpc) have affiliated C IV absorption; however, none (0/7) of the galaxies in denser regions show C IV. Similarly, the C IV detection rate is lower for galaxies residing in groups with dark matter halo masses of M [subscript halo] > 10[superscript12.5]M [subscript ⊙]. In contrast to C IV, H i is pervasive in the circumgalactic medium without regard to mass or environment. These results indicate that C IV absorbers with logN(C IV) ≳13.5 [superscript -2 cm] trace the halos of M* > 10 [superscript 9.5]M[subscript ⊙] galaxies but also reflect larger-scale environmental conditions.
Date issued
2016-11
URI
http://hdl.handle.net/1721.1/108168
Department
MIT Kavli Institute for Astrophysics and Space Research
Journal
The Astrophysical Journal
Publisher
IOP Publishing
Citation
Burchett, Joseph N., Todd M. Tripp, Rongmon Bordoloi, Jessica K. Werk, J. Xavier Prochaska, Jason Tumlinson, C. N. A. Willmer, John O’Meara, and Neal Katz. “A DEEP SEARCH FOR FAINT GALAXIES ASSOCIATED WITH VERY LOW REDSHIFT C Iv ABSORBERS. III. THE MASS- AND ENVIRONMENT-DEPENDENT CIRCUMGALACTIC MEDIUM.” The Astrophysical Journal 832, no. 2 (November 22, 2016): 124. © 2016 The American Astronomical Society
Version: Final published version
ISSN
1538-4357
0004-637X

Collections
  • MIT Open Access Articles

Browse

All of DSpaceCommunities & CollectionsBy Issue DateAuthorsTitlesSubjectsThis CollectionBy Issue DateAuthorsTitlesSubjects

My Account

Login

Statistics

OA StatisticsStatistics by CountryStatistics by Department
MIT Libraries
PrivacyPermissionsAccessibilityContact us
MIT
Content created by the MIT Libraries, CC BY-NC unless otherwise noted. Notify us about copyright concerns.