The X-ray structure of NGC 5128

Details The X-ray structure of NGC 5128 The X-ray structure of NGC 5128

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...219l..81d&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 219, Jan. 15, 1978, p. L81-L83. Research supported by the Massachuse

Astronomy and Astrophysics

Astronomy

35

Galactic Structure, Satellite Observation, X Ray Sources, Collimators, Galactic Radiation, Infrared Astronomy, Light Curve, Radio Sources (Astronomy), Sas

Scientific paper

During an observation of NGC 5128 (Cen A) by the rotating modulation collimator on board the SAS-3 X-ray observatory in early June 1975, data were obtained which suggest the presence of an extended source with about 3 arcmin FWHM surrounding an extremely compact object located at the radio/IR nucleus. The point component exhibited a 25% increase in intensity over a period of 2 to 5 hours.

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