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Discovery of an X-ray QSOThe discovery of X-ray QSO MR2251-178 at a distance of 410 Mpc is reported. The observations are based on signals (2-11 keV) from NRAO's Very Large Array (VLA) radio telescope and from two independent rotating modulation collimators (RMC). Coordinates are given and positional identification with X-ray source 2A2251-179 is made. Examination of POSS plates and redshift has given rise to speculation that MR2251-178 could actually be a Seyfert galaxy; but its high luminosity would tend to support the contention that it is, indeed, a QSO.
Document ID
19780036409
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ricker, G. R.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Clarke, 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.
(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 9, 2013
Publication Date
January 5, 1978
Publication Information
Publication: Nature
Volume: 271
Subject Category
Astronomy
Accession Number
78A20318
Funding Number(s)
CONTRACT_GRANT: NAS5-11450
Distribution Limits
Public
Copyright
Other

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