A narrrow-line radio galaxy behind the Fornax cluster

Details A narrrow-line radio galaxy behind the Fornax cluster A narrrow-line radio galaxy behind the Fornax cluster

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203p..49c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 203, June 1983, p. 49P-52P.

Astronomy and Astrophysics

Astronomy

9

Elliptical Galaxies, Emission Spectra, Galactic Clusters, Radio Galaxies, Seyfert Galaxies, Spectral Line Width, Centimeter Waves, Galactic Nuclei, Ionized Gases, Magnetohydrodynamic Turbulence, Radial Velocity

Scientific paper

The galaxy identified with the strongest component of the radio source PKS 0336-35 has a spectrum typical of narrow-line radio galaxies. The relative line strengths indicate that the lines come from a region of high ionization; linewidths indicate that the rms turbulent velocities in this region are <150 km s-1, somewhat low for this type of galaxy. The heliocentric radial velocity is 33750 ± 30 km s-1.

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