No evidence for a different accretion mode for all 3CR FR I radio galaxies
We have analyzed the optical and radio properties of a sample of 3CR FR I radio galaxies which have Hubble Space Telescope imaging capable of detecting optical cores. The jet powers of the FR I radio galaxies are estimated from their low-frequency radio luminosities, and the optical core luminosity...
| Main Authors: | , |
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| 格式: | Journal article |
| 出版: |
2003
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