Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31271
DC Field | Value | Language |
---|---|---|
dc.contributor.author | PAPITTO, ALESSANDRO | en_US |
dc.contributor.author | Falanga, M. | en_US |
dc.contributor.author | Hermsen, W. | en_US |
dc.contributor.author | MEREGHETTI, Sandro | en_US |
dc.contributor.author | Kuiper, L. | en_US |
dc.contributor.author | Poutanen, J. | en_US |
dc.contributor.author | Bozzo, E. | en_US |
dc.contributor.author | AMBROSINO, Filippo | en_US |
dc.contributor.author | Coti Zelati, F. | en_US |
dc.contributor.author | De Falco, V. | en_US |
dc.contributor.author | DE MARTINO, Domitilla | en_US |
dc.contributor.author | Di Salvo, T. | en_US |
dc.contributor.author | Esposito, P. | en_US |
dc.contributor.author | Ferrigno, C. | en_US |
dc.contributor.author | Forot, M. | en_US |
dc.contributor.author | Götz, D. | en_US |
dc.contributor.author | Gouiffes, C. | en_US |
dc.contributor.author | Iaria, R. | en_US |
dc.contributor.author | Laurent, P. | en_US |
dc.contributor.author | Li, J. | en_US |
dc.contributor.author | Li, Z. | en_US |
dc.contributor.author | MINEO, TERESA | en_US |
dc.contributor.author | Moran, P. | en_US |
dc.contributor.author | Neronov, A. | en_US |
dc.contributor.author | PAIZIS, ADAMANTIA | en_US |
dc.contributor.author | Rea, N. | en_US |
dc.contributor.author | Riggio, A. | en_US |
dc.contributor.author | SANNA, ALBERTO | en_US |
dc.contributor.author | Savchenko, V. | en_US |
dc.contributor.author | Słowikowska, A. | en_US |
dc.contributor.author | Shearer, A. | en_US |
dc.contributor.author | Tiengo, A. | en_US |
dc.contributor.author | Torres, D. F. | en_US |
dc.date.accessioned | 2021-12-28T12:18:03Z | - |
dc.date.available | 2021-12-28T12:18:03Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.issn | 1387-6473 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31271 | - |
dc.description.abstract | In the last 25 years a new generation of X-ray satellites imparted a significant leap forward in our knowledge of X-ray pulsars. The discovery of accreting and transitional millisecond pulsars proved that disk accretion can spin up a neutron star to a very high rotation speed. The detection of MeV-GeV pulsed emission from a few hundreds of rotation-powered pulsars probed particle acceleration in the outer magnetosphere, or even beyond. Also, a population of two dozens of magnetars has emerged. INTEGRAL played a central role to achieve these results by providing instruments with high temporal resolution up to the hard X-ray/soft, γ-ray band and a large field of view imager with good angular resolution to spot hard X-ray transients. In this article we review the main contributions by INTEGRAL to our understanding of the pulsating hard X-ray sky, such as the discovery and characterization of several accreting and transitional millisecond pulsars, the generation of the first catalog of hard X-ray/soft γ-ray rotation-powered pulsars, the detection of polarization in the hard X-ray emission from the Crab pulsar, and the discovery of persistent hard X-ray emission from several magnetars. | en_US |
dc.language.iso | eng | en_US |
dc.title | The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.newar.2020.101544 | en_US |
dc.identifier.scopus | 2-s2.0-85096659420 | en_US |
dc.identifier.isi | WOS:000598886100001 | en_US |
dc.identifier.url | http://arxiv.org/abs/2012.01346v1 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/abs/pii/S138764732030021X?via%3Dihub | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 91 | en_US |
dc.relation.firstpage | 101544 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | NEW ASTRONOMY REVIEWS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2020NewAR..9101544P | en_US |
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.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.dept | IASF Milano | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | IASF Palermo | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0001-6289-7413 | - |
crisitem.author.orcid | 0000-0003-3259-7801 | - |
crisitem.author.orcid | 0000-0001-7915-996X | - |
crisitem.author.orcid | 0000-0002-5069-4202 | - |
crisitem.author.orcid | 0000-0002-4931-8445 | - |
crisitem.author.orcid | 0000-0001-5067-0377 | - |
crisitem.author.orcid | 0000-0001-7960-4912 | - |
crisitem.journal.journalissn | 1387-6473 | - |
crisitem.journal.ance | E117454 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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2012.01346.pdf | preprint open access | 2.59 MB | Adobe PDF | View/Open |
2020-Papitto-NewAR-published.pdf | [Administrators only] | 6.46 MB | Adobe PDF |
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