CaltechAUTHORS
  A Caltech Library Service

Discovery of a probable binary quasar

Djorgovski, S. and Perley, R. and Meylan, G. and McCarthy, P. (1987) Discovery of a probable binary quasar. Astrophysical Journal, 321 . L17-L21. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20190805-085434845

[img] PDF (ADS) - Published Version
See Usage Policy.

639Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20190805-085434845

Abstract

We report discovery of a pair of quasars at a redshift of 1.345, separated by 4”.2 in projection, apparently associated with the radio source PKS 1145-071. The optical intensity ratio of the two images is approximately 2.5. The spectra are very similar, and all emission lines except for the C IV λI549 have the same equivalent widths, within the error bars. The redshift difference based on the C IV line alone, which is the strongest feature, and on the cross-correlation of the two spectra including the C IV line, is approximately 250 ± 100 km s^(-1) in the rest frame. If this discrepant emission line is excluded, the redshift difference drops to approximately 100 ± 100 km s^(-1), and is consistent with zero. Thus, on the basis of the optical data alone, we would have concluded that this double QSO is another example of gravitational lensing. However, the radio source is single and unresolved at all VLA frequencies, and positionally coincident with the brighter of the two optical images. The fainter of the two optical components is at least a factor of 500 fainter in the radio. This dramatic difference in L_(opt)/L_(radio) between the two components suggests that the system is a genuine binary quasar, and the first such well-documented case. Assuming that the two QSO’s are gravitationally bound, we derive a lower limit to the total mass of the system of ~ 10^(11)h^(-1)M_⊙ this is the first such direct determination of a quasar mass. The close projected separation of the pair (~ 20h^(-1) kpc) and the small velocity difference are suggestive of an interaction, which may be causally related to the QSO activity, and of the existence of a parent group or cluster, which would be a very interesting find in itself. In the view of this discovery, it is plausible that some other, previously reported gravitational lenses may be really pairs of physically distinct quasars.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/184998DOIArticle
ORCID:
AuthorORCID
Djorgovski, S.0000-0002-0603-3087
Additional Information:© 1987 The American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1987 May 8; accepted 1987 July 13. Based in part on observations made at the Multiple Mirror Telescope Observatory, a joint facility of the Smithsonian Institution and University of Arizona, and on observations made at the European Southern Observatory, La Silla, Chile. We would like to thank the staffs of MMT, ESO, and VLA observatories for their able help during our observing runs, and to John Huchra for the guidance at the MMT. We also thank Susan Tokarz for her help in MMT data reductions. Rudy Schild obtained some early CCD frames of the field. David Morabito kindly provided some unpublished information of the VLBI measurements. We acknowledge constructive comments of an anonymous referee. S. D. acknowledges a partial support from Harvard University.
Funders:
Funding AgencyGrant Number
Harvard UniversityUNSPECIFIED
Subject Keywords:gravitation — quasars — radio sources: general
Record Number:CaltechAUTHORS:20190805-085434845
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190805-085434845
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:97630
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:05 Aug 2019 16:11
Last Modified:03 Oct 2019 21:33

Repository Staff Only: item control page