Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31274
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | DE MARTINO, Domitilla | en_US |
dc.contributor.author | BERNARDINI, Federico | en_US |
dc.contributor.author | Mukai, K. | en_US |
dc.contributor.author | Falanga, M. | en_US |
dc.contributor.author | MASETTI, NICOLA | en_US |
dc.date.accessioned | 2021-12-28T12:27:07Z | - |
dc.date.available | 2021-12-28T12:27:07Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.issn | 0273-1177 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31274 | - |
dc.description.abstract | Among hard X-ray Galactic sources detected in the Swift and INTEGRAL surveys, those discovered as accreting white dwarf binaries have suprisingly boosted in number in the recent years. The majority are identified as magnetic Cataclysmic Variables of the Intermediate Polar type, suggesting this subclass as an important constituent of the Galactic population of X-ray sources. We here review and discuss the X-ray emission properties of newly discovered sources in the framework of an identification programme with the XMM-Newton satellite that increased the sample of this subclass by a factor of two. | en_US |
dc.language.iso | eng | en_US |
dc.title | Hard X-ray Cataclysmic Variables | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.asr.2019.09.006 | en_US |
dc.identifier.scopus | 2-s2.0-85073023781 | en_US |
dc.identifier.isi | 000551487800001 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/pii/S0273117719306544?via%3Dihub | en_US |
dc.identifier.url | http://arxiv.org/abs/1909.06306v1 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 66 | en_US |
dc.relation.issue | 5 | en_US |
dc.relation.firstpage | 1209 | en_US |
dc.relation.lastpage | 1225 | en_US |
dc.relation.numberofpages | 17 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 5 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | USA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ADVANCES IN SPACE RESEARCH | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2020AdSpR..66.1209D | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | 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. Capodimonte | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0002-5069-4202 | - |
crisitem.author.orcid | 0000-0001-5326-2010 | - |
crisitem.author.orcid | 0000-0001-9487-7740 | - |
crisitem.journal.journalissn | 0273-1177 | - |
crisitem.journal.ance | E003411 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
1909.06306.pdf | preprint | 608.52 kB | Adobe PDF | Visualizza/apri |
1-s2.0-S0273117719306544-main.pdf | [Administrators only] | 808.35 kB | Adobe PDF |
Page view(s)
55
controllato il 6-mag-2024
Download(s)
20
controllato il 6-mag-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.