X-RAY PROPERTIES OF THE NUCLEAR SOURCE IN THE CYGNUS A GALAXY

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Session 59 -- General Properties of AGN
Oral presentation, Tuesday, 10, 1995, 10:00am - 11:30am

[59.03] X-RAY PROPERTIES OF THE NUCLEAR SOURCE IN THE CYGNUS A GALAXY

D.E. Harris (SAO), R.A. Perley (NRAO), C.L. Carilli (Leiden, NL)

From a ROSAT HRI observation of Cygnus A (66 ksec), we find a second X-ray component approximately 5.5'' south-east of the nuclear source. We will discuss the relation of the source morphology to the optical and radio emission and evaluate the ``obscured quasar'' hypothesis for the nuclear emission on the basis of source intensity and limits to the variability.

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