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The cluster-scale environment of PKS 2155-304

Farina, E.; Fumagalli, M.; Decarli, R.; Fanidakis, N.

The cluster-scale environment of PKS 2155-304 Thumbnail


Authors

E. Farina

R. Decarli

N. Fanidakis



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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