Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34514
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Gnarini, A | en_US |
dc.contributor.author | Ursini, Francesco | en_US |
dc.contributor.author | Matt, G | en_US |
dc.contributor.author | Bianchi, S | en_US |
dc.contributor.author | CAPITANIO, FIAMMA | en_US |
dc.contributor.author | COCCHI, Massimo | en_US |
dc.contributor.author | FARINELLI, Ruben | en_US |
dc.contributor.author | Zhang, W | en_US |
dc.date.accessioned | 2024-01-09T13:50:05Z | - |
dc.date.available | 2024-01-09T13:50:05Z | - |
dc.date.issued | 2022 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/34514 | - |
dc.description.abstract | X-ray polarimetry missions like Imaging X-ray Polarimetry Explorer will be able to measure for the first time the polarization properties of accreting, weakly magnetized neutron stars in low-mass X-ray binaries. In this work, we present simulations of the expected X-ray polarized signal, including the coronal emission for different geometries of the corona itself, i.e. a slab above the accretion disc and a spherical shell around the neutron star. The simulations are performed with the fully relativistic Monte Carlo code MONK capable of computing the X-ray polarization degree and angle for various physical input parameters of the neutron star, disc, and corona. Different coronal geometries result in significantly different X-ray polarization properties, which can therefore be used to constrain the geometry of the systems. | en_US |
dc.language.iso | eng | en_US |
dc.title | Polarization properties of weakly magnetized neutron stars in low-mass X-ray binaries | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stac1523 | en_US |
dc.identifier.scopus | 2-s2.0-85133692086 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/514/2/2561/6598828 | en_US |
dc.identifier.url | http://arxiv.org/abs/2206.00749v1 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 514 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2561 | en_US |
dc.relation.lastpage | 2567 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2022MNRAS.514.2561G | 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 | IAPS Roma | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0001-9442-7897 | - |
crisitem.author.orcid | 0000-0002-6384-3027 | - |
crisitem.author.orcid | 0000-0002-5817-3129 | - |
crisitem.author.orcid | 0000-0003-2212-367X | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
stac1523.pdf | Pdf editoriale | 968.07 kB | Adobe PDF | View/Open |
2206.00749.pdf | preprint | 2.01 MB | Adobe PDF | View/Open |
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