FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2107582014> ?p ?o ?g. }

• W2107582014 endingPage "1161" @default.
• W2107582014 startingPage "1144" @default.
• W2107582014 abstract "We analysed the X-ray spectra of six observations, simultaneously taken with XMM-Newton and Rossi X-ray Timing Explorer (RXTE), of the neutron star low-mass X-ray binary 4U 1636-53. The observations cover several states of the source, and therefore a large range of inferred mass accretion rate. These six observations show a broad emission line in the spectrum at around 6.5 keV, likely due to iron. We fitted this line with a set of phenomenological models of a relativistically broadened line, plus a model that accounts for relativistically smeared and ionised reflection from the accretion disc. The latter model includes the incident emission from both the neutron-star surface or boundary layer and the corona that is responsible for the high-energy emission in these systems. From the fits with the reflection model we found that in four out of the six observations the main contribution to the reflected spectrum comes from the neutron-star surface or boundary layer, whereas in the other two observations the main contribution to the reflected spectrum comes from the corona. We found that the relative contribution of these two components is not correlated to the state of the source. From the phenomenological models we found that the iron line profile is better described by a symmetric, albeit broad, profile. The width of the line cannot be explained only by Compton broadening, and we therefore explored the case of relativistic broadening. We further found that the direct emission from the disc, boundary layer, and corona generally evolved in a manner consistent with the standard accretion disc model, with the disc and boundary layer becoming hotter and the disc moving inwards as the source changed from the hard in to the soft state. The iron line, however, did not appear to follow the same trend." @default.
• W2107582014 created "2016-06-24" @default.
• W2107582014 creator A5031287081 @default.
• W2107582014 creator A5031313316 @default.
• W2107582014 creator A5035495162 @default.
• W2107582014 creator A5050115215 @default.
• W2107582014 creator A5065960584 @default.
• W2107582014 creator A5082180400 @default.
• W2107582014 date "2013-04-28" @default.
• W2107582014 modified "2023-10-06" @default.
• W2107582014 title "Broad iron line in the fast spinning neutron-star system 4U 1636−53" @default.
• W2107582014 cites W122812805 @default.
• W2107582014 cites W1967757904 @default.
• W2107582014 cites W1991514755 @default.
• W2107582014 cites W2014475710 @default.
• W2107582014 cites W2027018483 @default.
• W2107582014 cites W2037978621 @default.
• W2107582014 cites W2040268062 @default.
• W2107582014 cites W2043384049 @default.
• W2107582014 cites W2043681094 @default.
• W2107582014 cites W2052669181 @default.
• W2107582014 cites W2073175230 @default.
• W2107582014 cites W2076672907 @default.
• W2107582014 cites W2078500152 @default.
• W2107582014 cites W2078742035 @default.
• W2107582014 cites W2088772258 @default.
• W2107582014 cites W2089770849 @default.
• W2107582014 cites W2090927807 @default.
• W2107582014 cites W2095576186 @default.
• W2107582014 cites W2105086180 @default.
• W2107582014 cites W2105356924 @default.
• W2107582014 cites W2107865293 @default.
• W2107582014 cites W2110097516 @default.
• W2107582014 cites W2113415740 @default.
• W2107582014 cites W2113417477 @default.
• W2107582014 cites W2120338534 @default.
• W2107582014 cites W2120656065 @default.
• W2107582014 cites W2124876248 @default.
• W2107582014 cites W2130351827 @default.
• W2107582014 cites W2153878267 @default.
• W2107582014 cites W2154078330 @default.
• W2107582014 cites W2159261874 @default.
• W2107582014 cites W2162470336 @default.
• W2107582014 cites W2163505141 @default.
• W2107582014 cites W3098472422 @default.
• W2107582014 cites W3098900157 @default.
• W2107582014 cites W3099357603 @default.
• W2107582014 cites W3099841661 @default.
• W2107582014 cites W3101049120 @default.
• W2107582014 cites W3101145576 @default.
• W2107582014 cites W3101222249 @default.
• W2107582014 cites W3102529193 @default.
• W2107582014 cites W3102843677 @default.
• W2107582014 cites W3102890407 @default.
• W2107582014 cites W3103223982 @default.
• W2107582014 cites W3103843170 @default.
• W2107582014 cites W3104701349 @default.
• W2107582014 cites W3104754302 @default.
• W2107582014 cites W3105091793 @default.
• W2107582014 cites W3105355850 @default.
• W2107582014 cites W3106330882 @default.
• W2107582014 cites W3123112321 @default.
• W2107582014 cites W3123658410 @default.
• W2107582014 cites W3124579176 @default.
• W2107582014 cites W3125033456 @default.
• W2107582014 cites W4232918148 @default.
• W2107582014 doi "https://doi.org/10.1093/mnras/stt530" @default.
• W2107582014 hasPublicationYear "2013" @default.
• W2107582014 type Work @default.
• W2107582014 sameAs 2107582014 @default.
• W2107582014 citedByCount "33" @default.
• W2107582014 countsByYear W21075820142013 @default.
• W2107582014 countsByYear W21075820142014 @default.
• W2107582014 countsByYear W21075820142015 @default.
• W2107582014 countsByYear W21075820142016 @default.
• W2107582014 countsByYear W21075820142017 @default.
• W2107582014 countsByYear W21075820142018 @default.
• W2107582014 countsByYear W21075820142019 @default.
• W2107582014 countsByYear W21075820142020 @default.
• W2107582014 countsByYear W21075820142021 @default.
• W2107582014 countsByYear W21075820142022 @default.
• W2107582014 countsByYear W21075820142023 @default.
• W2107582014 crossrefType "journal-article" @default.
• W2107582014 hasAuthorship W2107582014A5031287081 @default.
• W2107582014 hasAuthorship W2107582014A5031313316 @default.
• W2107582014 hasAuthorship W2107582014A5035495162 @default.
• W2107582014 hasAuthorship W2107582014A5050115215 @default.
• W2107582014 hasAuthorship W2107582014A5065960584 @default.
• W2107582014 hasAuthorship W2107582014A5082180400 @default.
• W2107582014 hasBestOaLocation W21075820141 @default.
• W2107582014 hasConcept C121332964 @default.
• W2107582014 hasConcept C1276947 @default.
• W2107582014 hasConcept C137179401 @default.
• W2107582014 hasConcept C192887742 @default.
• W2107582014 hasConcept C198352243 @default.
• W2107582014 hasConcept C199360897 @default.
• W2107582014 hasConcept C2524010 @default.
• W2107582014 hasConcept C2776401274 @default.

• next