Publication:
Synchrotron radiation from giant e ± pair halos

dc.contributor.authorA. Eungwanichayapanten_US
dc.contributor.authorW. Maithongen_US
dc.contributor.authorD. Ruffoloen_US
dc.contributor.otherMae Fah Luang Universityen_US
dc.contributor.otherMahidol Universityen_US
dc.contributor.otherThailand Center of Excellence in Physics (ThEP)en_US
dc.date.accessioned2018-05-03T08:43:55Z
dc.date.available2018-05-03T08:43:55Z
dc.date.issued2011-09-01en_US
dc.description.abstractA 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.en_US
dc.identifier.citationProceedings of the International Astronomical Union. Vol.7, No.S284 (2011), 417-419en_US
dc.identifier.doi10.1017/S1743921312009556en_US
dc.identifier.issn17439221en_US
dc.identifier.issn17439213en_US
dc.identifier.other2-s2.0-84865698859en_US
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/20.500.14594/12842
dc.rightsMahidol Universityen_US
dc.rights.holderSCOPUSen_US
dc.source.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84865698859&origin=inwarden_US
dc.subjectPhysics and Astronomyen_US
dc.titleSynchrotron radiation from giant e ± pair halosen_US
dc.typeConference Paperen_US
dspace.entity.typePublication
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84865698859&origin=inwarden_US

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