Orlando, E. (2017) High-energy and very-high-energy gamma-ray observations of the Milky Way. Il nuovo cimento C, 40 (3). pp. 1-6. ISSN 1826-9885
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Abstract
Observations of the gamma-ray emission from the Milky Way have significantly improved in recent years thanks to the current space instruments such as Fermi LAT and AGILE, and to the ground-based telescopes at higher energies such as for example H.E.S.S., VERITAS, MAGIC, and HAWC. While these high-quality data are providing crucial information on Galactic sources, interstellar emissions, and high-energy particles, they are challenging our understanding. I will discuss the state of the art, recent results, and prospects for future instruments.
Item Type: | Article |
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Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
Depositing User: | Marina Spanti |
Date Deposited: | 17 Nov 2020 09:51 |
Last Modified: | 17 Nov 2020 09:51 |
URI: | http://eprints.bice.rm.cnr.it/id/eprint/19943 |
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