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HEAO 1 observations of high-energy X-rays from the Seyfert I galaxy Mkn 509The results of observations of the Seyfert I galaxy Mkn 509 at high X-ray energies (14-140 keV) with the UCSD/MIT instrument aboard HEAO 1 are reported. The source is detected at energies above 40 keV, and the spectrum is consistent with an extrapolation of the power-law spectrum obtained at lower X-ray energies. Observations on four separate days in 1978 October indicate that the source is varying on a time scale of days.
Document ID
19820032823
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Dil, S.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Primini, F. A.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Bautz, M.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Howe, S. K.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Lang, F.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Levine, A. M.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Lewin, W. H. G.
(MIT Cambridge, MA, United States)
Worrall, D. M.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Nolan, P. L.
(California, University La Jolla, CA, United States)
Basinska, E.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Date Acquired
August 10, 2013
Publication Date
November 15, 1981
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
82A16358
Funding Number(s)
CONTRACT_GRANT: NAS8-27974
CONTRACT_GRANT: NAS8-27975
Distribution Limits
Public
Copyright
Other

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