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The parsec-scale central components of FRI radio galaxies

Abstract:

A majority of a complete sample of 3CR FR I radio galaxies show unresolved optical nuclear sources on the scales of 0.1 aresec. About half of the 3CR FR II radio galaxies observed with the HST also show Compact Central Cores (CCC). These CCCs have been interpreted as the optical counterparts of the non-thermal radio cores in these radio galaxies (Chiaberge, Capetti and Celotti 1999). We show that the optical flux density of the CCCs in FR Is is correlated with the radio core prominence. This ...

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Publication status:
Published

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Volume:
250
Pages:
100-103
Publication date:
2002-01-01
URN:
uuid:f18ecb0a-e61b-4eba-b0c7-70dad39c6579
Source identifiers:
27008
Local pid:
pubs:27008
ISBN:
1-58381-090-0
Keywords:

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