Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26644
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Archibald, R. F. | en_US |
dc.contributor.author | BURGAY, MARTA | en_US |
dc.contributor.author | Lyutikov, M. | en_US |
dc.contributor.author | Kaspi, V. M. | en_US |
dc.contributor.author | Esposito, P. | en_US |
dc.contributor.author | ISRAEL, Gian Luca | en_US |
dc.contributor.author | Kerr, M. | en_US |
dc.contributor.author | POSSENTI, ANDREA | en_US |
dc.contributor.author | Rea, N. | en_US |
dc.contributor.author | Sarkissian, J. | en_US |
dc.contributor.author | Scholz, P. | en_US |
dc.contributor.author | Tendulkar, S. P. | en_US |
dc.date.accessioned | 2020-07-27T09:44:33Z | - |
dc.date.available | 2020-07-27T09:44:33Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26644 | - |
dc.description.abstract | Rotation-powered pulsars and magnetars are two different observational manifestations of neutron stars: rotation-powered pulsars are rapidly spinning objects that are mostly observed as pulsating radio sources, while magnetars, neutron stars with the highest known magnetic fields, often emit short-duration X-ray bursts. Here, we report simultaneous observations of the high-magnetic-field radio pulsar PSR J1119-6127 at X-ray, with XMM-Newton and NuSTAR, and at radio energies with the Parkes radio telescope, during a period of magnetar-like bursts. The rotationally powered radio emission shuts off coincident with the occurrence of multiple X-ray bursts and recovers on a timescale of ∼70 s. These observations of related radio and X-ray phenomena further solidify the connection between radio pulsars and magnetars and suggest that the pair plasma produced in bursts can disrupt the acceleration mechanism of radio-emitting particles. | en_US |
dc.language.iso | eng | en_US |
dc.title | Magnetar-like X-Ray Bursts Suppress Pulsar Radio Emission | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/2041-8213/aa9371 | en_US |
dc.identifier.scopus | 2-s2.0-85034234867 | en_US |
dc.identifier.isi | 000414266100002 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/2041-8213/aa9371 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 849 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | L20 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017ApJ...849L..20A | 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 | 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. Cagliari | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0002-8265-4344 | - |
crisitem.author.orcid | 0000-0001-5480-6438 | - |
crisitem.author.orcid | 0000-0001-5902-3731 | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Archibald2017.pdf | Pdf editoriale | 617.57 kB | Adobe PDF | View/Open |
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