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Chandra Observations of the Nuclei of Radio Galaxies: 3C 295 and Hydra AThe angular resolution available with Chandra allows us to isolate the X-ray emission from the nucleus of many radio galaxies and obtain their spectra. As expected from unification schemes, spectra so far obtained can best be interpreted as heavily absorbed power laws. We present the spectral parameters so derived for 3C 295 and Hydra A and compare them to data obtained at other wavelengths.
Document ID
20000096515
Acquisition Source
Marshall Space Flight Center
Document Type
Abstract
Authors
Harris, D. E. (Smithsonian Astrophysical Observatory Cambridge, MA United States)
McNamara, B. R. (Smithsonian Astrophysical Observatory Cambridge, MA United States)
David, L. P. (Smithsonian Astrophysical Observatory Cambridge, MA United States)
Lavoie, Anthony R.
Date Acquired
August 19, 2013
Publication Date
January 1, 2000
Subject Category
Astronomy
Meeting Information
Meeting: 24th IAF General Assembly Meeting
Location: Manchester
Country: United Kingdom
Start Date: August 7, 2000
End Date: August 18, 2000
Funding Number(s)
CONTRACT_GRANT: NAS8-39073
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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