No evidence for a different accretion mode for all 3CR FR I radio galaxies
Open Access
- 21 April 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 349 (4) , 1419-1427
- https://doi.org/10.1111/j.1365-2966.2004.07608.x
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This publication has 61 references indexed in Scilit:
- Theory of the M 87 jetPublished by Springer Nature ,2007
- The Optically Powerful Quasar E1821+643 is Associated with a 300 Kiloparsec–Scale FR I Radio StructureThe Astrophysical Journal, 2001
- The Spectra and Energies of Classical Double Radio LobesThe Astronomical Journal, 2000
- The Blandford-Znajek Mechanism and the Emission from Isolated Accreting Black HolesThe Astrophysical Journal, 1999
- On the fate of gas accreting at a low rate on to a black holeMonthly Notices of the Royal Astronomical Society, 1999
- Turbulence and Angular Momentum Transport in a Global Accretion Disk SimulationThe Astrophysical Journal, 1998
- Relativistic Jets and the Fanaroff-Riley Classification of Radio GalaxiesThe Astrophysical Journal Supplement Series, 1995
- Toward Understanding the Fanaroff-Riley Dichotomy in Radio Source Morphology and PowerThe Astrophysical Journal, 1995
- Hydromagnetic flows from accretion discs and the production of radio jetsMonthly Notices of the Royal Astronomical Society, 1982
- Electromagnetic extraction of energy from Kerr black holesMonthly Notices of the Royal Astronomical Society, 1977