Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/30556
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | PITTORI, Carlotta | en_US |
dc.date.accessioned | 2021-02-23T12:25:36Z | - |
dc.date.available | 2021-02-23T12:25:36Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0218-2718 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30556 | - |
dc.description.abstract | We give an overview of the AGILE γ-ray satellite scientific highlights. AGILE is an Italian Space Agency (ASI) mission devoted to observations in the 30MeV-50GeV γ-ray energy range, with simultaneous X-ray imaging in the 18-60keV band. Launched in April 2007, the AGILE satellite has completed its tenth year of operations in orbit, and it is substantially contributing to improve our knowledge of the high-energy sky. Emission from cosmic sources at energies above 100MeV is intrinsically nonthermal, and the study of the wide variety of observed Galactic and extragalactic γ-ray sources provides a unique opportunity to test theories of particle acceleration and radiation processes in extreme conditions. | en_US |
dc.language.iso | eng | en_US |
dc.title | AGILE results on relativistic outflows above 100MeV | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1142/S0218271818440157 | en_US |
dc.identifier.scopus | 2-s2.0-85045475022 | en_US |
dc.identifier.isi | 000440352200016 | en_US |
dc.identifier.url | https://www.worldscientific.com/doi/pdf/10.1142/S0218271818440157 | en_US |
dc.identifier.url | https://arxiv.org/abs/2012.00156 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 27 | en_US |
dc.relation.issue | 10 | en_US |
dc.relation.firstpage | 1844015 | en_US |
dc.relation.numberofpages | 9 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 1 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | INTERNATIONAL JOURNAL OF MODERN PHYSICS D | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018IJMPD..2744015P | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.orcid | 0000-0001-6661-9779 | - |
crisitem.journal.journalissn | 0218-2718 | - |
crisitem.journal.ance | E085513 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
2012.00156.pdf | postprint | 2.95 MB | Adobe PDF | Visualizza/apri |
Page view(s)
52
controllato il 3-mag-2024
Download(s)
13
controllato il 3-mag-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.