Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26794
DC Field | Value | Language |
---|---|---|
dc.contributor.author | MEREGHETTI, Sandro | en_US |
dc.contributor.author | RIGOSELLI, MICHELA | en_US |
dc.date.accessioned | 2020-08-25T12:58:20Z | - |
dc.date.available | 2020-08-25T12:58:20Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0250-6335 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26794 | - |
dc.description.abstract | Observations obtained in the last years challenged the widespread notion that rotation-powered neutron stars are steady X-ray emitters. Besides a few allegedly rotation-powered neutron stars that showed `magnetar-like' variability, a particularly interesting case is that of PSR B0943+10. Recent observations have shown that this pulsar, well studied in the radio band where it alternates between a bright and a quiescent mode, displays significant X-ray variations, anticorrelated in flux with the radio emission. The study of such synchronous radio/X-ray mode switching opens a new window to investigate the processes responsible for the pulsar radio and high-energy emission. Here we review the main X-ray properties of PSR B0943+10 derived from recent coordinated X-ray and radio observations. | en_US |
dc.language.iso | eng | en_US |
dc.title | The Radio and X-ray Mode-Switching Pulsar PSR B0943+10 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s12036-017-9464-7 | en_US |
dc.identifier.scopus | 2-s2.0-85029508182 | en_US |
dc.identifier.isi | 000411868900019 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007%2Fs12036-017-9464-7 | en_US |
dc.identifier.url | https://arxiv.org/abs/1709.07233 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 38 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 54 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | no | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF ASTROPHYSICS AND ASTRONOMY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017JApA...38...54M | 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 | IASF Milano | - |
crisitem.author.orcid | 0000-0003-3259-7801 | - |
crisitem.journal.journalissn | 0250-6335 | - |
crisitem.journal.ance | E090630 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Mereghetti-Rigoselli2017_Article_TheRadioAndX-rayMode-Switching.pdf | Pdf editoriale | 837.02 kB | Adobe PDF | View/Open |
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