Prospects for Galactic transient sources detection with the Cherenkov Telescope Array
Prospects for Galactic transient sources detection with the Cherenkov Telescope Array
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Author / Creator
López-Oramas, A , Bulgarelli, A , Chaty, S , Chernyakova, M , Gnatyk, R , Hnatyk, B , Kantzas, D , Markoff, S , McKeague, S , Mereghetti, S , Mestre, E , A di Piano , Romano, P , Sadeh, I , Sergijenko, O , Sidoli, L , Spolon, A , E de Oña Wilhelmi , Piano, G and Zampieri, L
Publisher
Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Several types of Galactic sources, like magnetars, microquasars, novae or pulsar wind nebulae flares, display transient emission in the X-ray band. Some of these sources have also shown emission at MeV--GeV energies. However, none of these Galactic transients have ever been detected in the very-high-energy (VHE; E\(>\)100 GeV) regime by any Imaging...
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Full title
Prospects for Galactic transient sources detection with the Cherenkov Telescope Array
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TN_cdi_proquest_journals_2559946863
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2559946863
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2108.03911
