Amelia Fraser-McKelvie
The rarity of star formation in brightest cluster galaxies as measured by WISE
Fraser-McKelvie, Amelia; Brown, Michael J. I.; Pimbblet, Kevin A.
Authors
Abstract
We present the mid-infrared star formation rates of 245 X-ray selected, nearby (z < 0.1) brightest cluster galaxies (BCGs). A homogeneous and volume limited sample of BCGs was created by X-ray selecting clusters with Lx > 1 × 1044 erg s⁻ ¹. The Wide-Field Infrared Survey Explorer (WISE) All WISE Data Release provides the first measurement of the 12 μm star formation indicator for all BCGs in the nearby Universe. Perseus A and Cygnus A are the only galaxies in our sample to have star formation rates of > 40 M⊙ yr⁻¹, indicating that these two galaxies are highly unusual at current times. Stellar populations of 99 ± 0.6 per cent of local BCGs are (approximately) passively evolving, with star formation rates of < 10 M⊙ yr⁻¹. We find that in general, star formation produces only modest BCG growth at the current epoch.
Citation
Fraser-McKelvie, A., Brown, M. J. I., & Pimbblet, K. A. (2014). The rarity of star formation in brightest cluster galaxies as measured by WISE. Monthly notices of the Royal Astronomical Society. Letters, 444(1), L63-L67. https://doi.org/10.1093/mnrasl/slu117
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 18, 2014 |
Online Publication Date | Aug 12, 2014 |
Publication Date | Oct 11, 2014 |
Deposit Date | Jun 17, 2015 |
Publicly Available Date | Jun 17, 2015 |
Journal | Monthly notices of the Royal Astronomical Society Letters |
Electronic ISSN | 1745-3933 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 444 |
Issue | 1 |
Pages | L63-L67 |
DOI | https://doi.org/10.1093/mnrasl/slu117 |
Keywords | Galaxies -- clusters -- general; Galaxies -- elliptical and lenticular; cD; Galaxies -- star formation; Infrared -- galaxies |
Public URL | https://hull-repository.worktribe.com/output/375478 |
Publisher URL | http://mnrasl.oxfordjournals.org/content/444/1/L63.abstract |
Additional Information | This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Contract Date | Jun 17, 2015 |
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Copyright Statement
© 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society
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