Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23305
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Potekhin, Alexander Y. | en_US |
dc.contributor.author | DE LUCA, Andrea | en_US |
dc.contributor.author | Pons, José A. | en_US |
dc.date.accessioned | 2020-03-17T10:20:37Z | - |
dc.date.available | 2020-03-17T10:20:37Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 0038-6308 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23305 | - |
dc.description.abstract | Confronting theoretical models with observations of thermal radiation emitted by neutron stars is one of the most important ways to understand the properties of both, superdense matter in the interiors of the neutron stars and dense magnetized plasmas in their outer layers. Here we review the theory of thermal emission from the surface layers of strongly magnetized neutron stars, and the main properties of the observational data. In particular, we focus on the nearby sources for which a clear thermal component has been detected, without being contaminated by other emission processes (magnetosphere, accretion, nebulae). We also discuss the applications of the modern theoretical models of the formation of spectra of strongly magnetized neutron stars to the observed thermally emitting objects. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | Neutron Stars - Thermal Emitters | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s11214-014-0102-2 | en_US |
dc.identifier.scopus | 2-s2.0-84945441461 | en_US |
dc.identifier.isi | 000363722700006 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007%2Fs11214-014-0102-2 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 191 | en_US |
dc.relation.issue | 1-4 | en_US |
dc.relation.firstpage | 171 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | ESP | en_US |
dc.contributor.country | RUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | SPACE SCIENCE REVIEWS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2015SSRv..191..171P | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0038-6308 | - |
crisitem.journal.ance | E158291 | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0001-6739-687X | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1409.7666.pdf | postprint | 730.52 kB | Adobe PDF | View/Open |
Potekhin2015_Article_NeutronStarsThermalEmitters.pdf | [Administrators only] | 1.74 MB | Adobe PDF | View/Open |
Page view(s)
66
checked on Sep 12, 2024
Download(s)
48
checked on Sep 12, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.