Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31611
DC Field | Value | Language |
---|---|---|
dc.contributor.author | AMATO, Elena | en_US |
dc.contributor.author | Olmi, Barbara | en_US |
dc.date.accessioned | 2022-03-16T12:20:33Z | - |
dc.date.available | 2022-03-16T12:20:33Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 2218-1997 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31611 | - |
dc.description.abstract | Slightly more than 30 years ago, Whipple detection of the Crab Nebula was the start of Very High Energy gamma-ray astronomy. Since then, gamma-ray observations of this source have continued to provide new surprises and challenges to theories, with the detection of fast variability, pulsed emission up to unexpectedly high energy, and the very recent detection of photons with energy exceeding 1 PeV. In this article, we review the impact of gamma-ray observations on our understanding of this extraordinary accelerator. | en_US |
dc.language.iso | eng | en_US |
dc.title | The crab pulsar and nebula as seen in gamma-rays | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3390/universe7110448 | en_US |
dc.identifier.scopus | 2-s2.0-85121340226 | en_US |
dc.identifier.url | https://www.mdpi.com/2218-1997/7/11/448 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85121340226 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 7 | en_US |
dc.relation.issue | 11 | en_US |
dc.relation.firstpage | 448 | en_US |
dc.type.referee | REF_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 | UNIVERSE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_10 High energy and particle astronomy – X-rays, cosmic rays, gamma rays, neutrinos | 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.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 2218-1997 | - |
crisitem.journal.ance | E230956 | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-9881-8112 | - |
crisitem.author.orcid | 0000-0001-6022-8216 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
21Universe.pdf | PDF editoriale | 6.43 MB | Adobe PDF | View/Open |
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Items in DSpace are published in Open Access, unless otherwise indicated.