Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30278
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Li, Jian | en_US |
dc.contributor.author | Torres, Diego F. | en_US |
dc.contributor.author | Coti Zelati, Francesco | en_US |
dc.contributor.author | PAPITTO, ALESSANDRO | en_US |
dc.contributor.author | Kerr, Matthew | en_US |
dc.contributor.author | Rea, Nanda | en_US |
dc.date.accessioned | 2021-02-10T12:09:53Z | - |
dc.date.available | 2021-02-10T12:09:53Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 2041-8205 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30278 | - |
dc.description.abstract | Based on a theoretical selection of pulsars as candidates for detection at X-ray energies, we present an analysis of archival X-ray observations performed with Chandra and XMM-Newton of PSR J1747-2958 (the pulsar in the “Mouse” nebula), PSR J2021+3651 (the pulsar in the “Dragonfly” nebula), and PSR J1826-1256. X-ray pulsations from PSR J1747-2958 and PSR J1826-1256 are detected for the first time, and a previously reported hint of an X-ray pulsation from PSR J2021+3651 is confirmed with a higher significance. We analyze these pulsars’ spectra in regard to the theoretically predicted energy distribution, finding a remarkable agreement, and provide here a refined calculation of the model parameters taking into account the newly derived X-ray spectral data. | en_US |
dc.language.iso | eng | en_US |
dc.title | Theoretically Motivated Search and Detection of Non-thermal Pulsations from PSRs J1747-2958, J2021+3651, and J1826-1256 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/2041-8213/aae92b | en_US |
dc.identifier.scopus | 2-s2.0-85057876610 | en_US |
dc.identifier.isi | 000451002200006 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/2041-8213/aae92b | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 868 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | L29 | 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 LETTERS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018ApJ...868L..29L | en_US |
dc.relation.fund | H2020 | en_US |
dc.relation.project | TMSP (Mass accretion and ejection in transitional millisecond pulsars) | 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::PE9_10 High energy and particle astronomy – X-rays, cosmic rays, gamma rays, neutrinos | 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. Roma | - |
crisitem.author.orcid | 0000-0001-6289-7413 | - |
crisitem.project.grantno | 660657 | - |
crisitem.journal.journalissn | 2041-8205 | - |
crisitem.journal.ance | E196528 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Li_2018_ApJL_868_L29.pdf | Pdf editoriale | 1.34 MB | Adobe PDF | View/Open |
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