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Infrared observations of the X-ray quasars 0241 + 622 and MR2251–178

Soifer, B. T. and Neugebauer, G. and Matthews, K. (1979) Infrared observations of the X-ray quasars 0241 + 622 and MR2251–178. Nature, 278 (5701). pp. 231-232. ISSN 0028-0836. doi:10.1038/278231a0.

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Two new quasars have recently been found through X-ray observations (the only other one being 3C273, see refs 1, 2). Ricker et al. have reported observations confirming the identification of the X-ray source 2251–178 with a quasar of visual magnitude 14.1. Canizares, McClintock, and Ricker have reported visual spectrophotometric observations of this quasar, and find its visual spectrum is much like other low redshift quasars. Apparao et al. have reported the discovery of a low redshift quasar identified with the X-ray source 4U0241 + 61. Margon and Kwitter have reported detailed visual spectrophotometry of this quasar, 0241 + 622, and likewise find that its spectrum is typical of low redshift quasars. Because of the importance of establishing any morphologically unique characteristics of X-ray quasars, these quasars should be observed at all possible wavelengths. We report here IR observations of the two newly discovered X-ray quasars. These observations indicate that the X-ray quasars have IR properties typical of low redshift quasars, and, along with 3C273, are among the brightest known quasars at IR wavelengths.

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Additional Information:© 1979 Nature Publishing Group. Received 11 December 1978; accepted 31 January 1979. We thank G. Tuton and J. Carrasco for assistance with the observations. We also thank B. Margan for sending a preprint of his observations of 0241 + 622. This research was supported by NSF grant AST 77-20516 and NASA grant NGL 05-002-207.
Funding AgencyGrant Number
NSFAST 77-20516
NASANGL 05-002-207
Issue or Number:5701
Record Number:CaltechAUTHORS:20170228-091502830
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Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74584
Deposited By: Tony Diaz
Deposited On:28 Feb 2017 18:40
Last Modified:11 Nov 2021 05:28

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