Edward C. Moran
Published 2000-05-08Version 1
While NLS1s have been studied intensively at X-ray and optical wavelengths, comparatively little is known about their characteristics in the radio band. Therefore, we have carried out an investigation of the radio luminosities, source sizes, spectral index distribution, and variability of a large, uniformly selected sample of NLS1s. Our results indicate that, in some respects, the radio properties of NLS1s differ significantly from those of classical Seyfert galaxies. Radio observations of NLS1s may thus provide important clues regarding the nature of their nuclear activity.
Comments: Contributed talk presented at the Joint MPE,AIP,ESO workshop on NLS1s, Bad Honnef, Dec. 1999, to appear in New Astronomy Reviews; also available at http://wave.xray.mpe.mpg.de/conferences/nls1-workshop
Journal: New Astron.Rev. 44 (2000) 527-529
Radio Properties of z>4 Optically-Selected Quasars
The phase of the radio and X-ray pulses of PSR B1937+21
A population of high-redshift type-2 quasars-II. Radio Properties
