FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3099210321> ?p ?o ?g. }

• W3099210321 abstract "The Coma cluster was observed with an X-ray Imaging Spectrometer (XIS) onboard Suzaku in six pointings, including the central X-ray peak region, the 14'west offset region, 30'and 34'north-west offset regions, and 44'and 60'south-west offset regions. Owing to its lower background level, Suzaku has better sensitivity to Fe K-alpha lines than other satellites. Using precise Fe line measurements, we studied the temperature structure, possible bulk motions, and iron abundance distributions in the intracluster medium (ICM). The observed spectra were well-represented by a single-temperature model, and two- or three- temperature model did not improve chi-square substantially. The temperature, derived from K-alpha line ratios of H-like and He-like Fe, agree with those derived from the single-temperature model. Because the line ratio is a steep function of temperature, the consistency supports the accuracy of temperature measurements conducted with Suzaku. Within the 34'region, the redshift derived from the central energy of the He-like Fe line is consistent with that from optical observations, within a calibration error of 18 eV or 818 km/s in the line of sight. This value is smaller than the sound velocity of ICM, which is 1500 km/s. The central energy of Fe lines at the 44'offset region around the NGC 4839 subcluster is also consistent with those within the 34'region. These results on the temperature and velocity structure suggest that the core of the cluster is in a relaxed state, and non-thermal electrons relevant to the radio halo are accelerated by intracluster turbulence rather than large-scale shocks. Fe abundance is almost constant at 0.4 solar within the 34'region, and decreases with radius. This value is slightly lower than those of other clusters, which means the gas have been mixed well during a past merger associated with the growth of the cluster." @default.
• W3099210321 created "2020-11-23" @default.
• W3099210321 creator A5003751526 @default.
• W3099210321 creator A5008122738 @default.
• W3099210321 creator A5012635295 @default.
• W3099210321 creator A5018475424 @default.
• W3099210321 creator A5051483967 @default.
• W3099210321 creator A5060262806 @default.
• W3099210321 date "2011-11-25" @default.
• W3099210321 modified "2023-10-05" @default.
• W3099210321 title "Suzaku Observations of Iron K-Lines from the Intracluster Medium of the Coma Cluster" @default.
• W3099210321 cites W1500596920 @default.
• W3099210321 cites W1520358395 @default.
• W3099210321 cites W1665336903 @default.
• W3099210321 cites W1729839103 @default.
• W3099210321 cites W184963066 @default.
• W3099210321 cites W1964078714 @default.
• W3099210321 cites W1968473807 @default.
• W3099210321 cites W1972431651 @default.
• W3099210321 cites W1975215917 @default.
• W3099210321 cites W1977362570 @default.
• W3099210321 cites W1978316006 @default.
• W3099210321 cites W1986879811 @default.
• W3099210321 cites W1987848293 @default.
• W3099210321 cites W1994772731 @default.
• W3099210321 cites W1996610606 @default.
• W3099210321 cites W1996758820 @default.
• W3099210321 cites W1997089041 @default.
• W3099210321 cites W2002941573 @default.
• W3099210321 cites W2009031292 @default.
• W3099210321 cites W2010438020 @default.
• W3099210321 cites W2025489111 @default.
• W3099210321 cites W2026370807 @default.
• W3099210321 cites W2030221216 @default.
• W3099210321 cites W2037216179 @default.
• W3099210321 cites W2045016983 @default.
• W3099210321 cites W2054489755 @default.
• W3099210321 cites W2058024252 @default.
• W3099210321 cites W2059887224 @default.
• W3099210321 cites W2064598581 @default.
• W3099210321 cites W2071758179 @default.
• W3099210321 cites W2074852325 @default.
• W3099210321 cites W2083643586 @default.
• W3099210321 cites W2088515199 @default.
• W3099210321 cites W2091456938 @default.
• W3099210321 cites W2096471541 @default.
• W3099210321 cites W2115003665 @default.
• W3099210321 cites W2125603840 @default.
• W3099210321 cites W2126688676 @default.
• W3099210321 cites W2141623727 @default.
• W3099210321 cites W2146318694 @default.
• W3099210321 cites W2150479035 @default.
• W3099210321 cites W2166504775 @default.
• W3099210321 cites W2170408727 @default.
• W3099210321 cites W3016007611 @default.
• W3099210321 cites W3098418583 @default.
• W3099210321 cites W3099001851 @default.
• W3099210321 cites W3099966559 @default.
• W3099210321 cites W3100195645 @default.
• W3099210321 cites W3102016691 @default.
• W3099210321 cites W3102277392 @default.
• W3099210321 cites W3102295407 @default.
• W3099210321 cites W3102531267 @default.
• W3099210321 cites W3103241715 @default.
• W3099210321 cites W3103444911 @default.
• W3099210321 cites W3104114621 @default.
• W3099210321 cites W3104372594 @default.
• W3099210321 cites W3105022426 @default.
• W3099210321 cites W3122798494 @default.
• W3099210321 cites W4292403095 @default.
• W3099210321 cites W4301003189 @default.
• W3099210321 doi "https://doi.org/10.1093/pasj/63.sp3.s991" @default.
• W3099210321 hasPublicationYear "2011" @default.
• W3099210321 type Work @default.
• W3099210321 sameAs 3099210321 @default.
• W3099210321 citedByCount "22" @default.
• W3099210321 countsByYear W30992103212012 @default.
• W3099210321 countsByYear W30992103212013 @default.
• W3099210321 countsByYear W30992103212014 @default.
• W3099210321 countsByYear W30992103212015 @default.
• W3099210321 countsByYear W30992103212016 @default.
• W3099210321 countsByYear W30992103212017 @default.
• W3099210321 countsByYear W30992103212018 @default.
• W3099210321 countsByYear W30992103212019 @default.
• W3099210321 countsByYear W30992103212020 @default.
• W3099210321 countsByYear W30992103212021 @default.
• W3099210321 crossrefType "journal-article" @default.
• W3099210321 hasAuthorship W3099210321A5003751526 @default.
• W3099210321 hasAuthorship W3099210321A5008122738 @default.
• W3099210321 hasAuthorship W3099210321A5012635295 @default.
• W3099210321 hasAuthorship W3099210321A5018475424 @default.
• W3099210321 hasAuthorship W3099210321A5051483967 @default.
• W3099210321 hasAuthorship W3099210321A5060262806 @default.
• W3099210321 hasBestOaLocation W30992103211 @default.
• W3099210321 hasConcept C100893083 @default.
• W3099210321 hasConcept C121332964 @default.
• W3099210321 hasConcept C1276947 @default.
• W3099210321 hasConcept C147120987 @default.
• W3099210321 hasConcept C156055797 @default.
• W3099210321 hasConcept C164866538 @default.

• next