학술논문

The faint radio source population at 15.7 GHz – IV. The dominance of core emission in faint radio galaxies.
Document Type
Article
Source
Monthly Notices of the Royal Astronomical Society. Apr2020, Vol. 493 Issue 2, p2841-2853. 13p.
Subject
*RADIO galaxies
*SHORTWAVE radio
*DEMOGRAPHIC surveys
*RADIO frequency
*RADIOS
Language
ISSN
0035-8711
Abstract
We present 15-GHz Karl G. Jansky Very Large Array observations of a complete sample of radio galaxies selected at 15.7 GHz from the Tenth Cambridge (10C) survey. 67 out of the 95 sources (71 per cent) are unresolved in the new observations and lower frequency radio observations, placing an upper limit on their angular size of ∼2 arcsec. Thus, compact radio galaxies, or radio galaxies with very faint jets, are the dominant population in the 10C survey. This provides support for the suggestion in our previous work that low-luminosity (⁠|$L\lt 10^{25} \, \textrm{W~Hz}^{-1}$|⁠) radio galaxies are core dominated, although higher resolution observations are required to confirm this directly. The 10C sample of compact, high-frequency selected radio galaxies is a mixture of high-excitation and low-excitation radio galaxies and displays a range of radio spectral shapes, demonstrating that they are a mixed population of objects. [ABSTRACT FROM AUTHOR]