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pro vyhledávání: '"Summerlin, Errol J."'
Akademický článek
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Diffusive shock acceleration (DSA) at relativistic shocks is widely thought to be an important acceleration mechanism in various astrophysical jet sources, including radio-loud active galactic nuclei such as blazars. Such acceleration can produce the
Externí odkaz:
http://arxiv.org/abs/1609.03899
Diffusive shock acceleration (DSA) at relativistic shocks is likely to be an important acceleration mechanism in various astrophysical jet sources, including radio-loud AGN. An important recent development for blazar science is the ability of Fermi-L
Externí odkaz:
http://arxiv.org/abs/1312.3458
Diffusive shock acceleration (DSA) at relativistic shocks is expected to be an important acceleration mechanism in a variety of astrophysical objects including extragalactic jets in active galactic nuclei and gamma ray bursts. These sources remain go
Externí odkaz:
http://arxiv.org/abs/1110.5968
Publikováno v:
AIP Conf.Proc.1183:74-84,2009
Diffusive shock acceleration (DSA) at relativistic shocks is expected to be an important acceleration mechanism in a variety of astrophysical objects including extragalactic jets in active galactic nuclei and gamma ray bursts. These sources remain st
Externí odkaz:
http://arxiv.org/abs/0910.1072
Akademický článek
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Publikováno v:
AIP Conf.Proc.1039:240-245,2008
The acceleration of interstellar pick-up ions as well as solar wind species has been observed at a multitude of interplanetary (IP) shocks by different spacecraft. This paper expands upon previous work modeling the phase space distributions of accele
Externí odkaz:
http://arxiv.org/abs/0807.0934
Publikováno v:
Astrophys.J.667:L29-L32,2007
The observed spectra of blazars, their intrinsic emission, and the underlying populations of radiating particles are intimately related. The use of these sources as probes of the extragalactic infrared background, a prospect propelled by recent advan
Externí odkaz:
http://arxiv.org/abs/0707.4676
Publikováno v:
Astrophys.SpaceSci.307:165-168,2007
Recent advances in the understanding of the properties of supernova remnant shocks have been precipitated by the Chandra and XMM X-ray Observatories, and the HESS Atmospheric Cerenkov Telescope in the TeV band. A critical problem for this field is th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0609407
Heliospheric shocks are excellent systems for testing theories of particle acceleration in their environs. These generally fall into two classes: (1) interplanetary shocks that are linear in their ion acceleration characteristics, with the non-therma
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506179