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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Main Authors: A. Eungwanichayapant, W. Maithong, D. Ruffolo
Other Authors: Mae Fah Luang University
Format: Conference or Workshop Item
Published: 2018
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Online Access:https://repository.li.mahidol.ac.th/handle/123456789/12842
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spelling 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
institution Mahidol University
building Mahidol University Library
continent Asia
country Thailand
Thailand
content_provider Mahidol University Library
collection Mahidol University Institutional Repository
topic Physics and Astronomy
spellingShingle Physics and Astronomy
A. Eungwanichayapant
W. Maithong
D. Ruffolo
Synchrotron radiation from giant e ± pair halos
description 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.
author2 Mae Fah Luang University
author_facet Mae Fah Luang University
A. Eungwanichayapant
W. Maithong
D. Ruffolo
format Conference or Workshop Item
author A. Eungwanichayapant
W. Maithong
D. Ruffolo
author_sort 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
title_full_unstemmed Synchrotron radiation from giant e ± pair halos
title_sort synchrotron radiation from giant e ± pair halos
publishDate 2018
url https://repository.li.mahidol.ac.th/handle/123456789/12842
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