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Observations of an X-ray QSOThis paper reports X-ray, optical, radio, and IR measurements of the z = 0.068 QSO MR2251-178, which was initially discovered on the basis of its X-ray emission. Data are provided on the position, optical colors, and 2-10-keV X-ray luminosity of this low-redshift QSO. An absolute V magnitude of -24.2 is implied, and the X-ray/optical luminosity ratio is estimated to be about 3:1 at peak X-ray brightness. It is shown that the optical spectrum of MR2251-178 is quite normal for a QSO, except for an extremely broad H-alpha emission line with a FWZI of 30,000 to 40,000 km/s. The overall spectrum of MR2251-178 from the radio to the X-ray region is plotted, and the photometric history of this QSO since 1889 is briefly discussed.
Document ID
19800029234
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Ricker, G. R.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Clark, G. W.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Doxsey, R. E.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Dower, R. G.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Jernigan, J. G.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Canizares, C. R.
(MIT Cambridge, Mass., United States)
Delvaille, J. P.
(Smithsonian Astrophysical Observatory Cambridge, Mass., United States)
Macalpine, G. M.
(Michigan, University Ann Arbor, Mich., United States)
Hjellming, R. M.
(National Radio Astronomy Observatory Socorro, N. Mex., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Subject Category
Astrophysics
Meeting Information
Meeting: X-ray astronomy
Location: Innsbruck
Country: Austria
Start Date: May 29, 1978
End Date: June 10, 1978
Accession Number
80A13404
Funding Number(s)
CONTRACT_GRANT: NAS5-11450
Distribution Limits
Public
Copyright
Other

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