10 pages, 4 figures, to be published in the Astrophysical Journal ...
Prajval Shastri, Preeti Kharb
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Ultrahigh-energy cosmic rays from Fanaroff Riley class II radio galaxies
AIP Conference Proceedings, 1992The hot spots of Fanaroff Riley class II radio galaxies are argued to be the sources of the ultrahigh energy component in cosmic rays. We present calculations of cosmic ray transport in an evolving universe, taking the losses against the microwave background properly into account.
Jörg Rachen, Peter L. Biermann
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ROTATION MEASURES ACROSS PARSEC-SCALE JETS OF FANAROFF–RILEY TYPE I RADIO GALAXIES [PDF]
We present the results of a parsec-scale polarization study of three FRI radio galaxies—3C66B, 3C78, and 3C264—obtained with Very Long Baseline Interferometry at 5, 8, and 15 GHz. Parsec-scale polarization has been detected in a large number of beamed radio-loud active galactic nuclei, but in only a handful of the relatively unbeamed radio galaxies. We
Prajval Shastri, Preeti Kharb
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Classification of Fanaroff-Riley Radio Galaxies using Conventional Machine Learning Techniques
2019 International Multidisciplinary Information Technology and Engineering Conference (IMITEC), 2019Large scale radio astronomy projects such as the Square Kilometre Array (SKA) is expected to produce extremely large data sets (300 PB p/a), which makes purely manual classification no longer a viable option. An automatic method of radio galaxy classification is proposed in this paper that will examine the performance of conventional classification ...
Burger Becker, Trienko Grobler
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Fanaroff-Riley I galaxies as the parent populations of BL Lacertae objects. III - Radio constraints
Meg Urry, Paolo Padovani
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Dust in BL Lac objects and Fanaroff-Riley radio galaxies: infrared region
Astrophysics and Space Science, 2015Here 28 BL Lac objects, 18 FR I type radio galaxies, 4 FR I/II type radio galaxies and 10 FR II type radio galaxies are studied from FIR (far infrared) to optical region (180 μm to 0.44 μm) to understand the nature of infrared emission from these objects and the physical properties of dust in the emitting region.
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A physically-motivated perspective of Fanaroff–Riley classification of radio galaxies
Journal of Astrophysics and Astronomy, 2023null Gopal-Krishna +3 more
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The role of Fanaroff-Riley II radio galaxies in the acceleration of the most energetic cosmic rays
Nuclear Physics B - Proceedings Supplements, 2007Possible sources of ultra-high energy cosmic rays are the hot-spots of Fanaroff-Riley II radio galaxies. In fact, these regions meet the requirements of size, magnetic field intensity and presence of strong shocks for accelerating particles up to energies that exceed 10 21 eV . On the other hand, the interaction with the photons of the Cosmic
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Bayesian inference of jet bulk-flow speeds in Fanaroff-Riley type II radio sources
Monthly Notices of the Royal Astronomical Society, 2009Martin J. Hardcastle
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The prevalence of Fanaroff-Riley type I radio quasars
Monthly Notices of the Royal Astronomical Society, 2007Ian Heywood +2 more
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