The nature of the optical filaments in Centaurus A - Evidence for a beamed ionizing continuum

Astronomy and Astrophysics – Astronomy

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Active Galactic Nuclei, Photoionization, Radio Galaxies, Blazars, Brightness Distribution, Centaurus Constellation, Emission Spectra, Radiation Distribution, Radio Jets (Astronomy)

Scientific paper

Visible-band observations of the radio galaxy Cen A are reported. Data from long-slit 360-700-nm spectroscopy obtained with the B&C and EFOSC spectrographs on the 3.6-m telescope at ESO during 1987 and 1989, an R-band image obtained with the AAT, and forbidden O III (5007-A) images obtained with the EFOSC in March 1989 are presented and discussed in detail. The line-emitting filaments of the optical jet are found to have a complex structure with variation on 100-pc scales and no forbidden O III emission from the 'inner' or 'counter' jets. It is inferred that radiation from a nuclear continuum source (rendered invisible by obscuration and/or intrinsic anisotropy; e.g., relativistic beaming in the direction of the optical jet) is responsible for the photoionization of the filaments.

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