X-ray emission from Centaurus A

Details X-ray emission from Centaurus A X-ray emission from Centaurus A

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984xue..conf..102t&link_type=abstract

In Max-Planck Inst. für Physik und Astrophysik X-Ray and UV Emission from Active Galactic Nuclei p 102-104 (SEE N85-17790 08-88)

Astronomy and Astrophysics

Astronomy

1

Centaurus Constellation, Emission Spectra, Radio Galaxies, Vela Satellites, X Ray Spectra, Galactic Nuclei, Luminous Intensity, Periodic Variations, X Ray Astronomy

Scientific paper

The X-ray strength of Cen A (NGC 5128) was monitored for 10 yr by Vela
5B, beginning in 1969. The 1973-1975 period of exceptional activity and
strength was especially well covered. It is characterized by numerous
rapid changes in intensity, in agreement with other data, indicating
that the nucleus of Cen A is small but massive.

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