Synchrotron radiation from giant e ± pair halos
A giant e ± pair halo is formed by electromagnetic cascades developing around an AGN under the intergalactic magnetic field (1nG-1μG). Many studies have been focussed on the pair halos in the gamma band because it has been predicted that the e ± s in the pair halos up-scatter the Cosmic Microwave Ba...
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th-mahidol.128422018-05-03T15:43:55Z Synchrotron radiation from giant e ± pair halos A. Eungwanichayapant W. Maithong D. Ruffolo Mae Fah Luang University Mahidol University Thailand Center of Excellence in Physics (ThEP) Physics and Astronomy A giant e ± pair halo is formed by electromagnetic cascades developing around an AGN under the intergalactic magnetic field (1nG-1μG). Many studies have been focussed on the pair halos in the gamma band because it has been predicted that the e ± s in the pair halos up-scatter the Cosmic Microwave Background (CMB) to be gamma-rays. However, the pair halos do not emit only gamma photons but also X-ray photons via synchrotron radiation. In this paper, the Spectral Energy Distributions (SEDs) and the angular distributions of the synchrotron radiation of the pair halos from the Monte Carlo simulations will be discussed. © 2012 International Astronomical Union. 2018-05-03T08:43:55Z 2018-05-03T08:43:55Z 2011-09-01 Conference Paper Proceedings of the International Astronomical Union. Vol.7, No.S284 (2011), 417-419 10.1017/S1743921312009556 17439221 17439213 2-s2.0-84865698859 https://repository.li.mahidol.ac.th/handle/123456789/12842 Mahidol University SCOPUS https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84865698859&origin=inward |
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Physics and Astronomy A. Eungwanichayapant W. Maithong D. Ruffolo Synchrotron radiation from giant e ± pair halos |
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A giant e ± pair halo is formed by electromagnetic cascades developing around an AGN under the intergalactic magnetic field (1nG-1μG). Many studies have been focussed on the pair halos in the gamma band because it has been predicted that the e ± s in the pair halos up-scatter the Cosmic Microwave Background (CMB) to be gamma-rays. However, the pair halos do not emit only gamma photons but also X-ray photons via synchrotron radiation. In this paper, the Spectral Energy Distributions (SEDs) and the angular distributions of the synchrotron radiation of the pair halos from the Monte Carlo simulations will be discussed. © 2012 International Astronomical Union. |
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Mae Fah Luang University |
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Mae Fah Luang University A. Eungwanichayapant W. Maithong D. Ruffolo |
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Conference or Workshop Item |
author |
A. Eungwanichayapant W. Maithong D. Ruffolo |
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A. Eungwanichayapant |
title |
Synchrotron radiation from giant e ± pair halos |
title_short |
Synchrotron radiation from giant e ± pair halos |
title_full |
Synchrotron radiation from giant e ± pair halos |
title_fullStr |
Synchrotron radiation from giant e ± pair halos |
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Synchrotron radiation from giant e ± pair halos |
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synchrotron radiation from giant e ± pair halos |
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2018 |
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https://repository.li.mahidol.ac.th/handle/123456789/12842 |
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