Abstract
The authors present radio observations of a hard X-ray selected sample
of active galaxies, made with the VLA and Parkes radio telescopes. All
of the galaxies observed with the VLA were detected, making this an
excellent sample with which to look at the relationship between the
radio and X-ray emission from active galaxies. The authors use the ratio
of the radio to X-ray flux density as a measure of the degree of
"radio-loudness" of an active galaxy. They find no evidence for distinct
"radio-quiet" and "radio-loud" populations, rather there is a continuous
distribution of the degree of radio-loudness amongst the sample
galaxies. The X-ray and radio luminosity are found to be correlated. The
correlation is not linear, the radio-loud objects all having high X-ray
luminosity.
| Original language | English |
|---|---|
| Pages (from-to) | 521-531 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 228 |
| DOIs | |
| Publication status | Published - 1 Sept 1987 |
Keywords / Materials (for Non-textual outputs)
- Active Galaxies
- Astronomical Spectroscopy
- Galactic Structure
- Radiant Flux Density
- Radio Spectra
- X Ray Spectra
- Emission Spectra
- Spectrum Analysis
- Very Large Array (Vla)
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