FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2486367777> ?p ?o ?g. }

• W2486367777 endingPage "1863" @default.
• W2486367777 startingPage "1847" @default.
• W2486367777 abstract "On 2015 June 15, the black hole X-ray binary V404 Cygni went into outburst, exhibiting extreme X-ray variability which culminated in a final flare on June 26. Over the following days, the Swift-X-ray Telescope detected a series of bright rings, comprising five main components that expanded and faded with time, caused by X-rays scattered from the otherwise unobservable dust layers in the interstellar medium in the direction of the source. Simple geometrical modelling of the rings’ angular evolution reveals that they have a common temporal origin, coincident with the final, brightest flare seen by INTEGRAL's JEM X-1, which reached a 3–10 keV flux of ∼25 Crab. The high quality of the data allows the dust properties and density distribution along the line of sight to the source to be estimated. Using the Rayleigh–Gans approximation for the dust scattering cross-section and a power-law distribution of grain sizes a, ∝ a−q, the average dust emission is well modelled by |$q = 3.90^{+0.09}_{-0.08}$| and maximum grain size of |$a_+ = 0.147^{+0.024}_{-0.004} {rm mu m}$|⁠, though significant variations in q are seen between the rings. The recovered dust density distribution shows five peaks associated with the dense sheets responsible for the rings at distances ranging from 1.19 to 2.13 kpc, with thicknesses of ∼40–80 pc and a maximum density occurring at the location of the nearest sheet. We find a dust column density of Ndust ≈ (2.0–2.5) × 1011 cm−2, consistent with the optical extinction to the source. Comparison of the inner rings’ azimuthal X-ray evolution with archival Wide-field Infrared Survey Explorer mid-IR data suggests that the second most distant ring follows the general IR emission trend, which increases in brightness towards the Galactic north side of the source." @default.
• W2486367777 created "2016-08-23" @default.
• W2486367777 creator A5009220087 @default.
• W2486367777 creator A5011358663 @default.
• W2486367777 creator A5013690309 @default.
• W2486367777 creator A5023584585 @default.
• W2486367777 creator A5037047393 @default.
• W2486367777 creator A5040131259 @default.
• W2486367777 creator A5060680432 @default.
• W2486367777 creator A5065960584 @default.
• W2486367777 date "2016-07-22" @default.
• W2486367777 modified "2023-10-18" @default.
• W2486367777 title "Lord of the Rings – Return of the King:<i>Swift</i>-XRT observations of dust scattering rings around V404 Cygni" @default.
• W2486367777 cites W151596575 @default.
• W2486367777 cites W1882454150 @default.
• W2486367777 cites W1897059644 @default.
• W2486367777 cites W1937581169 @default.
• W2486367777 cites W1962131278 @default.
• W2486367777 cites W1964712402 @default.
• W2486367777 cites W1965372241 @default.
• W2486367777 cites W1968457280 @default.
• W2486367777 cites W1968761599 @default.
• W2486367777 cites W1987319691 @default.
• W2486367777 cites W1988538716 @default.
• W2486367777 cites W1992824168 @default.
• W2486367777 cites W1996932215 @default.
• W2486367777 cites W2000274354 @default.
• W2486367777 cites W2001977925 @default.
• W2486367777 cites W2004646985 @default.
• W2486367777 cites W2010671365 @default.
• W2486367777 cites W2013528275 @default.
• W2486367777 cites W2014649600 @default.
• W2486367777 cites W2015890794 @default.
• W2486367777 cites W2029343094 @default.
• W2486367777 cites W2034608771 @default.
• W2486367777 cites W2036422398 @default.
• W2486367777 cites W2041661662 @default.
• W2486367777 cites W2052937506 @default.
• W2486367777 cites W2060298912 @default.
• W2486367777 cites W2066068540 @default.
• W2486367777 cites W2067025050 @default.
• W2486367777 cites W2071647169 @default.
• W2486367777 cites W2111817932 @default.
• W2486367777 cites W2122342311 @default.
• W2486367777 cites W2123267088 @default.
• W2486367777 cites W2147476946 @default.
• W2486367777 cites W2155421027 @default.
• W2486367777 cites W2171074980 @default.
• W2486367777 cites W2287777434 @default.
• W2486367777 cites W2346246548 @default.
• W2486367777 cites W3022265438 @default.
• W2486367777 cites W3083094549 @default.
• W2486367777 cites W3098217400 @default.
• W2486367777 cites W3099830973 @default.
• W2486367777 cites W3101823059 @default.
• W2486367777 cites W3102087921 @default.
• W2486367777 cites W3102107381 @default.
• W2486367777 cites W3103843170 @default.
• W2486367777 cites W3104363485 @default.
• W2486367777 cites W3105377513 @default.
• W2486367777 cites W3106253105 @default.
• W2486367777 cites W3123112321 @default.
• W2486367777 cites W3124038249 @default.
• W2486367777 cites W4292403095 @default.
• W2486367777 doi "https://doi.org/10.1093/mnras/stw1753" @default.
• W2486367777 hasPublicationYear "2016" @default.
• W2486367777 type Work @default.
• W2486367777 sameAs 2486367777 @default.
• W2486367777 citedByCount "15" @default.
• W2486367777 countsByYear W24863677772017 @default.
• W2486367777 countsByYear W24863677772018 @default.
• W2486367777 countsByYear W24863677772019 @default.
• W2486367777 countsByYear W24863677772020 @default.
• W2486367777 countsByYear W24863677772023 @default.
• W2486367777 crossrefType "journal-article" @default.
• W2486367777 hasAuthorship W2486367777A5009220087 @default.
• W2486367777 hasAuthorship W2486367777A5011358663 @default.
• W2486367777 hasAuthorship W2486367777A5013690309 @default.
• W2486367777 hasAuthorship W2486367777A5023584585 @default.
• W2486367777 hasAuthorship W2486367777A5037047393 @default.
• W2486367777 hasAuthorship W2486367777A5040131259 @default.
• W2486367777 hasAuthorship W2486367777A5060680432 @default.
• W2486367777 hasAuthorship W2486367777A5065960584 @default.
• W2486367777 hasBestOaLocation W24863677771 @default.
• W2486367777 hasConcept C120665830 @default.
• W2486367777 hasConcept C121332964 @default.
• W2486367777 hasConcept C191486275 @default.
• W2486367777 hasConcept C191897082 @default.
• W2486367777 hasConcept C192562407 @default.
• W2486367777 hasConcept C2779588948 @default.
• W2486367777 hasConcept C2780928442 @default.
• W2486367777 hasConcept C44870925 @default.
• W2486367777 hasConcept C68709404 @default.
• W2486367777 hasConceptScore W2486367777C120665830 @default.
• W2486367777 hasConceptScore W2486367777C121332964 @default.
• W2486367777 hasConceptScore W2486367777C191486275 @default.
• W2486367777 hasConceptScore W2486367777C191897082 @default.
• W2486367777 hasConceptScore W2486367777C192562407 @default.

• next