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- Publisher Website: 10.1016/j.crhy.2015.09.001
- Scopus: eid_2-s2.0-84944447966
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Article: Gamma rays from the Galactic Centre region
Title | Gamma rays from the Galactic Centre region |
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Authors | |
Keywords | Fermi bubbles |
Issue Date | 2015 |
Citation | Comptes Rendus Physique, 2015, v. 16, n. 6-7, p. 686-703 How to Cite? |
Abstract | © 2015.During the last decades, increasingly precise astronomical observations of the Galactic Centre region at radio, infrared, and X-ray wavelengths laid the foundations for a detailed understanding of the high-energy astroparticle physics of this most remarkable location in the Galaxy. Recently, observations of this region in high energy (HE, 10 MeV-100 GeV) and very high energy (VHE, >100 GeV) γ-rays added important insights into the emerging picture of the Galactic nucleus as a most violent and active region where acceleration of particles to highest energies and their transport can be studied in great detail. We review the current understanding of the γ-ray emission emanating from the Galactic Centre. |
Persistent Identifier | http://hdl.handle.net/10722/226723 |
ISSN | 2023 Impact Factor: 1.3 2023 SCImago Journal Rankings: 0.448 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Su, Meng | - |
dc.contributor.author | van Eldik, Christopher | - |
dc.date.accessioned | 2016-06-29T01:58:24Z | - |
dc.date.available | 2016-06-29T01:58:24Z | - |
dc.date.issued | 2015 | - |
dc.identifier.citation | Comptes Rendus Physique, 2015, v. 16, n. 6-7, p. 686-703 | - |
dc.identifier.issn | 1631-0705 | - |
dc.identifier.uri | http://hdl.handle.net/10722/226723 | - |
dc.description.abstract | © 2015.During the last decades, increasingly precise astronomical observations of the Galactic Centre region at radio, infrared, and X-ray wavelengths laid the foundations for a detailed understanding of the high-energy astroparticle physics of this most remarkable location in the Galaxy. Recently, observations of this region in high energy (HE, 10 MeV-100 GeV) and very high energy (VHE, >100 GeV) γ-rays added important insights into the emerging picture of the Galactic nucleus as a most violent and active region where acceleration of particles to highest energies and their transport can be studied in great detail. We review the current understanding of the γ-ray emission emanating from the Galactic Centre. | - |
dc.language | eng | - |
dc.relation.ispartof | Comptes Rendus Physique | - |
dc.subject | Fermi bubbles | - |
dc.title | Gamma rays from the Galactic Centre region | - |
dc.type | Article | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1016/j.crhy.2015.09.001 | - |
dc.identifier.scopus | eid_2-s2.0-84944447966 | - |
dc.identifier.volume | 16 | - |
dc.identifier.issue | 6-7 | - |
dc.identifier.spage | 686 | - |
dc.identifier.epage | 703 | - |
dc.identifier.isi | WOS:000365244800008 | - |
dc.identifier.issnl | 1631-0705 | - |