FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2890946065> ?p ?o ?g. }

• W2890946065 endingPage "4122" @default.
• W2890946065 startingPage "4111" @default.
• W2890946065 abstract "We have initiated a programme to study the physical/dynamical state of gas in galaxy clusters and the impact of the cluster environment on gaseous halos of individual galaxies using X-ray imaging and UV absorption line spectroscopy of background QSOs. Here we report results from the analysis Chandra and XMM-Newton archival data of five galaxy clusters with such QSOs, one of which has an archival UV spectrum. We characterize the gravitational masses and dynamical states, as well as the hot intracluster medium (ICM) properties of these clusters. Most clusters are dynamically disturbed clusters based on the X-ray morphology parameters, the X-ray temperature profiles, the large offset between X-ray peak and brightest cluster galaxy (BCG). The baryon contents in the hot ICM and stars of these clusters within $r_{500}$ are lower than the values expected from the gravitational masses, according to the standard cosmology. We also estimate column densities of the hot ICM along the sightlines toward the background QSOs as well as place upper limits on the warm-hot phase for the one sightline with existing UV observations. These column densities, compared with those of the warm and warm-hot ICM to be measured with UV absorption line spectroscopy, will enable us to probe the relationship among various gaseous phases and their connection to the heating/cooling and dynamical processes of the clusters. Furthermore, our analysis of the archival QSO spectrum probing one cluster underscores the need for high quality, targeted UV observations to robustly constrain the 10$^{5-6}$ K gas phase." @default.
• W2890946065 created "2018-09-27" @default.
• W2890946065 creator A5013135871 @default.
• W2890946065 creator A5013194814 @default.
• W2890946065 creator A5036321241 @default.
• W2890946065 creator A5039259392 @default.
• W2890946065 creator A5041908392 @default.
• W2890946065 creator A5063485373 @default.
• W2890946065 creator A5064996219 @default.
• W2890946065 creator A5070153617 @default.
• W2890946065 date "2018-09-13" @default.
• W2890946065 modified "2023-10-14" @default.
• W2890946065 title "Probing the dynamical state, baryon content, and multiphase nature of galaxy clusters with bright background QSOs" @default.
• W2890946065 cites W1487294478 @default.
• W2890946065 cites W1609730404 @default.
• W2890946065 cites W1739534413 @default.
• W2890946065 cites W1826320254 @default.
• W2890946065 cites W1966667130 @default.
• W2890946065 cites W1967766027 @default.
• W2890946065 cites W1990523382 @default.
• W2890946065 cites W2001666843 @default.
• W2890946065 cites W2002438643 @default.
• W2890946065 cites W2010438020 @default.
• W2890946065 cites W2023541500 @default.
• W2890946065 cites W2032627363 @default.
• W2890946065 cites W2034255160 @default.
• W2890946065 cites W2036422398 @default.
• W2890946065 cites W2037009808 @default.
• W2890946065 cites W2038143200 @default.
• W2890946065 cites W2039862412 @default.
• W2890946065 cites W2047002529 @default.
• W2890946065 cites W2064895468 @default.
• W2890946065 cites W2068529188 @default.
• W2890946065 cites W2068618869 @default.
• W2890946065 cites W2073083682 @default.
• W2890946065 cites W2074987412 @default.
• W2890946065 cites W2082316064 @default.
• W2890946065 cites W2083908030 @default.
• W2890946065 cites W2084461563 @default.
• W2890946065 cites W2093808381 @default.
• W2890946065 cites W2098764133 @default.
• W2890946065 cites W2110205213 @default.
• W2890946065 cites W2111852396 @default.
• W2890946065 cites W2112736043 @default.
• W2890946065 cites W2115326311 @default.
• W2890946065 cites W2118950764 @default.
• W2890946065 cites W2120944638 @default.
• W2890946065 cites W2124499858 @default.
• W2890946065 cites W2124598998 @default.
• W2890946065 cites W2124733136 @default.
• W2890946065 cites W2129300743 @default.
• W2890946065 cites W2132936425 @default.
• W2890946065 cites W2145095123 @default.
• W2890946065 cites W2145122729 @default.
• W2890946065 cites W2152443818 @default.
• W2890946065 cites W2160791189 @default.
• W2890946065 cites W2162333545 @default.
• W2890946065 cites W2167562984 @default.
• W2890946065 cites W2185905637 @default.
• W2890946065 cites W2293962467 @default.
• W2890946065 cites W2612977727 @default.
• W2890946065 cites W2616080569 @default.
• W2890946065 cites W2899497983 @default.
• W2890946065 cites W3098326871 @default.
• W2890946065 cites W3098495404 @default.
• W2890946065 cites W3098803289 @default.
• W2890946065 cites W3100514957 @default.
• W2890946065 cites W3101374472 @default.
• W2890946065 cites W3101728524 @default.
• W2890946065 cites W3101832938 @default.
• W2890946065 cites W3102051593 @default.
• W2890946065 cites W3102904458 @default.
• W2890946065 cites W3103465215 @default.
• W2890946065 cites W3103555914 @default.
• W2890946065 cites W3105626659 @default.
• W2890946065 cites W3106249226 @default.
• W2890946065 cites W4289781552 @default.
• W2890946065 cites W4295989202 @default.
• W2890946065 doi "https://doi.org/10.1093/mnras/sty2492" @default.
• W2890946065 hasPublicationYear "2018" @default.
• W2890946065 type Work @default.
• W2890946065 sameAs 2890946065 @default.
• W2890946065 citedByCount "5" @default.
• W2890946065 countsByYear W28909460652019 @default.
• W2890946065 countsByYear W28909460652021 @default.
• W2890946065 countsByYear W28909460652022 @default.
• W2890946065 countsByYear W28909460652023 @default.
• W2890946065 crossrefType "journal-article" @default.
• W2890946065 hasAuthorship W2890946065A5013135871 @default.
• W2890946065 hasAuthorship W2890946065A5013194814 @default.
• W2890946065 hasAuthorship W2890946065A5036321241 @default.
• W2890946065 hasAuthorship W2890946065A5039259392 @default.
• W2890946065 hasAuthorship W2890946065A5041908392 @default.
• W2890946065 hasAuthorship W2890946065A5063485373 @default.
• W2890946065 hasAuthorship W2890946065A5064996219 @default.
• W2890946065 hasAuthorship W2890946065A5070153617 @default.
• W2890946065 hasBestOaLocation W28909460652 @default.
• W2890946065 hasConcept C100893083 @default.

• next