FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2892667252> ?p ?o ?g. }

• W2892667252 endingPage "A126" @default.
• W2892667252 startingPage "A126" @default.
• W2892667252 abstract "We report the results provided by the XMM-Newton observation of the X-ray binary pulsar SXP59.0 during its most recent outburst in April 2017. The source was detected at f X (0.2–12 keV) = 8 × 10 −11 erg cm −2 s −1 , one of its highest flux levels reported to date. The measured pulse period was P spin = 58.949(1) s, very similar to the periods measured in most of the previous observations. The pulsed emission was clearly detected over the whole energy range between 0.2 and 12 keV, but the pulse profile is energy dependent and the pulsed fraction increases as the energy increases. Although the time-averaged EPIC spectrum is dominated by a power-law component (with photon index Γ = 0.76 ± 0.01), the data show an evident soft excess, which can be described with the sum of a black-body and a hot thermal plasma component (with temperatures kT BB = 171 +11 −14 eV and kT APEC = 1.09 +0.16 −0.09 keV, respectively). Moreover, the EPIC and RGS spectra show narrow emission lines due to N, O, Ne, Mg, and Fe. The phase-resolved spectral analysis of the EPIC data shows that the flux of the black-body component varies with the pulse phase, while the plasma component is almost constant. We show that the black-body component can be attributed to the reprocessing of the primary emission by the optically thick material at the inner edge of the accretion disc, while the hot plasma component is due to a diffuse gas far from the accretion region and the narrow emission lines of the RGS spectrum are most probably due to photoionized matter around the accreting source." @default.
• W2892667252 created "2018-10-05" @default.
• W2892667252 creator A5001646931 @default.
• W2892667252 creator A5014665960 @default.
• W2892667252 creator A5016012032 @default.
• W2892667252 creator A5020987575 @default.
• W2892667252 creator A5031649360 @default.
• W2892667252 creator A5053839279 @default.
• W2892667252 date "2018-11-01" @default.
• W2892667252 modified "2023-10-09" @default.
• W2892667252 title "Spectral analysis of SXP59.0 during its 2017 outburst and properties of the soft excess in X-ray binary pulsars" @default.
• W2892667252 cites W1757987097 @default.
• W2892667252 cites W1910448147 @default.
• W2892667252 cites W1977829169 @default.
• W2892667252 cites W2014186817 @default.
• W2892667252 cites W2017878144 @default.
• W2892667252 cites W2023600253 @default.
• W2892667252 cites W2027802133 @default.
• W2892667252 cites W2052926897 @default.
• W2892667252 cites W2056299947 @default.
• W2892667252 cites W2060787233 @default.
• W2892667252 cites W2067899408 @default.
• W2892667252 cites W2070958830 @default.
• W2892667252 cites W2074867124 @default.
• W2892667252 cites W2082929737 @default.
• W2892667252 cites W2092375607 @default.
• W2892667252 cites W2095541289 @default.
• W2892667252 cites W2105903052 @default.
• W2892667252 cites W2154078330 @default.
• W2892667252 cites W2599377499 @default.
• W2892667252 cites W2778891751 @default.
• W2892667252 cites W3099875688 @default.
• W2892667252 cites W3100546802 @default.
• W2892667252 cites W3101347870 @default.
• W2892667252 cites W3101630617 @default.
• W2892667252 cites W3101907996 @default.
• W2892667252 cites W3103843170 @default.
• W2892667252 cites W3104812503 @default.
• W2892667252 cites W3105146472 @default.
• W2892667252 cites W3123112321 @default.
• W2892667252 doi "https://doi.org/10.1051/0004-6361/201833907" @default.
• W2892667252 hasPublicationYear "2018" @default.
• W2892667252 type Work @default.
• W2892667252 sameAs 2892667252 @default.
• W2892667252 citedByCount "2" @default.
• W2892667252 countsByYear W28926672522019 @default.
• W2892667252 countsByYear W28926672522021 @default.
• W2892667252 crossrefType "journal-article" @default.
• W2892667252 hasAuthorship W2892667252A5001646931 @default.
• W2892667252 hasAuthorship W2892667252A5014665960 @default.
• W2892667252 hasAuthorship W2892667252A5016012032 @default.
• W2892667252 hasAuthorship W2892667252A5020987575 @default.
• W2892667252 hasAuthorship W2892667252A5031649360 @default.
• W2892667252 hasAuthorship W2892667252A5053839279 @default.
• W2892667252 hasBestOaLocation W28926672521 @default.
• W2892667252 hasConcept C110363677 @default.
• W2892667252 hasConcept C120665830 @default.
• W2892667252 hasConcept C121332964 @default.
• W2892667252 hasConcept C12287442 @default.
• W2892667252 hasConcept C127413603 @default.
• W2892667252 hasConcept C1276947 @default.
• W2892667252 hasConcept C137179401 @default.
• W2892667252 hasConcept C153385146 @default.
• W2892667252 hasConcept C157909335 @default.
• W2892667252 hasConcept C178802073 @default.
• W2892667252 hasConcept C185544564 @default.
• W2892667252 hasConcept C191897082 @default.
• W2892667252 hasConcept C192562407 @default.
• W2892667252 hasConcept C192887742 @default.
• W2892667252 hasConcept C199364081 @default.
• W2892667252 hasConcept C2776401274 @default.
• W2892667252 hasConcept C42061751 @default.
• W2892667252 hasConcept C44870925 @default.
• W2892667252 hasConcept C4839761 @default.
• W2892667252 hasConcept C68709404 @default.
• W2892667252 hasConcept C82706917 @default.
• W2892667252 hasConcept C98444146 @default.
• W2892667252 hasConceptScore W2892667252C110363677 @default.
• W2892667252 hasConceptScore W2892667252C120665830 @default.
• W2892667252 hasConceptScore W2892667252C121332964 @default.
• W2892667252 hasConceptScore W2892667252C12287442 @default.
• W2892667252 hasConceptScore W2892667252C127413603 @default.
• W2892667252 hasConceptScore W2892667252C1276947 @default.
• W2892667252 hasConceptScore W2892667252C137179401 @default.
• W2892667252 hasConceptScore W2892667252C153385146 @default.
• W2892667252 hasConceptScore W2892667252C157909335 @default.
• W2892667252 hasConceptScore W2892667252C178802073 @default.
• W2892667252 hasConceptScore W2892667252C185544564 @default.
• W2892667252 hasConceptScore W2892667252C191897082 @default.
• W2892667252 hasConceptScore W2892667252C192562407 @default.
• W2892667252 hasConceptScore W2892667252C192887742 @default.
• W2892667252 hasConceptScore W2892667252C199364081 @default.
• W2892667252 hasConceptScore W2892667252C2776401274 @default.
• W2892667252 hasConceptScore W2892667252C42061751 @default.
• W2892667252 hasConceptScore W2892667252C44870925 @default.
• W2892667252 hasConceptScore W2892667252C4839761 @default.
• W2892667252 hasConceptScore W2892667252C68709404 @default.
• W2892667252 hasConceptScore W2892667252C82706917 @default.

• next