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4U0241+61 - A luminous low-redshift QSOThe faint (1.8 micro Jy, 2-11 keV) X-ray QSO 4U0241+61 is considered in terms of its celestial position (galactic latitude = +2.4 plus or minus 30 sec), luminosity (M sub v = -25.8 plus or minus 1.8), redshift (z = 0.0438), and radio emission (0.2-0.5 Jy). Counting rates in two energy channels are presented, and found comparable to the Type 1 Seyfert 3C120. Spectrophotometric calibration to an approximately 8 A resolution was also achieved. Attention is given to the close relation between X-ray emitting QSOs and Seyferts.
Document ID
19780055478
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Apparao, K. M. V.
(Tata Institute of Fundamental Research Bombay, India)
Bignami, G. F.
(Tata Inst. of Fundamental Research Bombay, India)
Maraschi, L.
(CNR Laboratorio di Fisica Cosmica e Technologie Relative, Milan, Italy)
Helmken, H.
(Harvard College Observatory and Smithsonian Astrophysical Observatory, Center for Astrophysics, Cambridge Mass., United States)
Margon, B.
(California, University Los Angeles, Calif., United States)
Hjellming, R.
(National Radio Astronomy Observatory Socorro, N. Mex., United States)
Bradt, H. V.
(Tata Inst. of Fundamental Research Bombay, India)
Dower, R. G.
(MIT Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
June 8, 1978
Publication Information
Publication: Nature
Volume: 273
Subject Category
Astrophysics
Accession Number
78A39387
Funding Number(s)
CONTRACT_GRANT: NAS5-11450
Distribution Limits
Public
Copyright
Other

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