CaltechAUTHORS
  A Caltech Library Service

Discovery of a Probable Physical Triple Quasar

Djorgovski, S. G. and Courbin, F. and Meylan, G. and Sluse, D. and Thompson, D. and Mahabal, A. and Glikman, E. (2007) Discovery of a Probable Physical Triple Quasar. Astrophysical Journal, 662 (1). L1-L5. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20091113-105347141

[img]
Preview
PDF - Published Version
See Usage Policy.

195Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20091113-105347141

Abstract

We report the discovery of the first known probable case of a physical triple quasar. A previously known double system, QQ 1429-008 at z = 2.076, is shown to contain a third, fainter QSO component at the same redshift. Deep optical and IR imaging has failed to reveal a plausible lensing galaxy group or a cluster, and we are unable to construct any viable lensing model that could lead to the observed distribution of source positions and relative intensities of the three QSO image components. There are also hints of differences in the broadband spectral energy distributions of the different components, which are more naturally understood if they are physically distinct active galactic nuclei (AGNs). Therefore, we conclude that this system is most likely a physical triple quasar, the first such close QSO grouping known at any redshift. The projected component separations are ~30-50 kpc, typical of interacting galaxy systems. The existence of this highly unusual system supports the standard picture in which galaxy interactions lead to the onset of QSO activity.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/519162 DOIArticle
http://www.iop.org/EJ/abstract/1538-4357/662/1/L1/PublisherArticle
ORCID:
AuthorORCID
Djorgovski, S. G.0000-0002-0603-3087
Sluse, D.0000-0001-6116-2095
Mahabal, A.0000-0003-2242-0244
Glikman, E.0000-0003-0489-3750
Additional Information:© 2007 The American Astronomical Society. Received 2006 December 22; accepted 2007 April 25; published 2007 May 22. We are grateful to the staff of the W. M. Keck and ESO-VLT observatories for their expert assistance in the course of our observing runs, and to M. Pahre with assistance from some of the Keck observations. The Keck data used in this Letter were obtained in a collaborative project involving J. Cohen, B. T. Soifer, R. Blandford, G. Neugebauer, and I. Smail. S. G. D., A. M., and E. G. acknowledge partial support from NSF grant AST-0407448 and from the Ajax Foundation. F. C., G. M., and D. S. are financially supported by the Swiss National Science Foundation (SNSF). S. G. D. acknowledges the hospitality of EPFL and the Geneva Observatory, where some of this work was performed.
Funders:
Funding AgencyGrant Number
NSFAST-0407448
Ajax FoundationUNSPECIFIED
Swiss National Science Foundation (SNSF)UNSPECIFIED
Subject Keywords:galaxies : interactions; gravitational lensing; quasars : general
Issue or Number:1
Record Number:CaltechAUTHORS:20091113-105347141
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20091113-105347141
Official Citation:Discovery of a Probable Physical Triple Quasar S. G. Djorgovski, F. Courbin, G. Meylan, D. Sluse, D. Thompson, A. Mahabal, and E. Glikman 2007 ApJ 662 L1-L5 doi: 10.1086/519162
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:16699
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Nov 2009 20:16
Last Modified:09 Mar 2020 13:19

Repository Staff Only: item control page