E. Farina
The cluster-scale environment of PKS 2155-304
Farina, E.; Fumagalli, M.; Decarli, R.; Fanidakis, N.
Authors
Abstract
PKS 2155−304 is one of the brightest extragalactic source in the X-ray and EUV bands, and is a prototype for the BL Lac class of objects. In this paper, we investigate the large-scale environment of this source using new multi-object as well as long-slit spectroscopy, together with archival spectra and optical images. We find clear evidence of a modest overdensity of galaxies at z = 0.116 10 ± 0.000 06, consistent with previous determinations of the BL Lac redshift. The galaxy group has a radial velocity dispersion of 250+80−40 km s−1 and a virial radius of 0.22 Mpc, yielding a role-of-thumb estimate of the virial mass of Mvir ∼ 1.5 × 1013 M⊙, i.e. one order of magnitude less than that observed in similar objects. This result hints towards a relatively wide diversity in the environmental properties of BL Lac objects.
Citation
Farina, E., Fumagalli, M., Decarli, R., & Fanidakis, N. (2016). The cluster-scale environment of PKS 2155-304. Monthly Notices of the Royal Astronomical Society, 455(1), 618-625. https://doi.org/10.1093/mnras/stv2277
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 28, 2015 |
Online Publication Date | Nov 5, 2015 |
Publication Date | Jan 1, 2016 |
Deposit Date | Nov 22, 2015 |
Publicly Available Date | Nov 23, 2015 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 455 |
Issue | 1 |
Pages | 618-625 |
DOI | https://doi.org/10.1093/mnras/stv2277 |
Keywords | BL Lacertae objects: individual: PKS 2155−304, Galaxies: groups: general. |
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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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