Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23628
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Gelfand, J. | en_US |
dc.contributor.author | Breton, R. | en_US |
dc.contributor.author | Ng, C. -Y. | en_US |
dc.contributor.author | Hessels, J. | en_US |
dc.contributor.author | Stappers, B. | en_US |
dc.contributor.author | Roberts, M. | en_US |
dc.contributor.author | POSSENTI, ANDREA | en_US |
dc.date.accessioned | 2020-03-27T08:57:44Z | - |
dc.date.available | 2020-03-27T08:57:44Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.isbn | 9781909204706 | en_US |
dc.identifier.issn | 1824-8039 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23628 | - |
dc.description.abstract | Neutron stars lose the bulk of their rotational energy in the form of a pulsar wind: an ultra-relativistic outflow of predominantly electrons and positrons. This pulsar wind significantly impacts the environment and possible binary companion of the neutron star, and studying the resultant pulsar wind nebulae is critical for understanding the formation of neutron stars and millisecond pulsars, the physics of the neutron star magnetosphere, the acceleration of leptons up to PeV energies, and how these particles impact the interstellar medium. With the SKA1 and the SKA2, it could be possible to study literally hundreds of PWNe in detail, critical for understanding the many open questions in the topics listed above. | en_US |
dc.language.iso | eng | en_US |
dc.title | Pulsar Wind Nebulae in the SKA era | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.22323/1.215.0046 | en_US |
dc.identifier.url | https://pos.sissa.it/215/046 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 215 | en_US |
dc.relation.firstpage | 46 | en_US |
dc.type.referee | REF_4 | en_US |
dc.description.numberofauthors | 7 | en_US |
dc.description.international | sì | en_US |
dc.relation.ispartofbook | Advancing Astrophysics with the Square Kilometre Array (AASKA14) | en_US |
dc.relation.conferencename | Advancing Astrophysics with the Square Kilometre Array (AASKA14) | en_US |
dc.relation.conferenceplace | Giardini Naxos, Italy | en_US |
dc.relation.conferencedate | 9 -13 June, 2014 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | POS PROCEEDINGS OF SCIENCE | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2015aska.confE..46G | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_6 Stars and stellar systems | 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 | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0001-5902-3731 | - |
crisitem.journal.journalissn | 1824-8039 | - |
crisitem.journal.ance | E188909 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
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AASKA14_046.pdf | PDF editoriale | 1.45 MB | Adobe PDF | View/Open |
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