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• W2118601380 endingPage "A105" @default.
• W2118601380 startingPage "A105" @default.
• W2118601380 abstract "We present relations between X-ray luminosity and velocity dispersion (L-sigma), X-ray luminosity and gas mass (L-Mgas), and cluster radius and velocity dispersion (r500-sigma) for 62 galaxy clusters in the HIFLUGCS, an X-ray flux-limited sample minimizing bias toward any cluster morphology. Our analysis in total is based on ~1.3Ms of clean X-ray XMM-Newton data and 13439 cluster member galaxies with redshifts. Cool cores are among the major contributors to the scatter in the L-sigma relation. When the cool-core-corrected X-ray luminosity is used the intrinsic scatter decreases to 0.27 dex. Even after the X-ray luminosity is corrected for the cool core, the scatter caused by the presence of cool cores dominates for the low-mass systems. The scatter caused by the non-cool-core clusters does not strongly depend on the mass range, and becomes dominant in the high-mass regime. The observed L-sigma relation agrees with the self-similar prediction, matches that of a simulated sample with AGN feedback disregarding six clusters with <45 cluster members with spectroscopic redshifts, and shows a common trend of increasing scatter toward the low-mass end, i.e., systems with sigma<500km/s. A comparison of observations with simulations indicates an AGN-feedback-driven impact in the low-mass regime. The best fits to the $L-M_{rm gas}$ relations for the disturbed clusters and undisturbed clusters in the observational sample closely match those of the simulated samples with and without AGN feedback, respectively. This suggests that one main cause of the scatter is AGN activity providing feedback in different phases, e.g., during a feedback cycle. The slope and scatter in the observed r500-sigma relation is similar to that of the simulated sample with AGN feedback except for a small offset but still within the scatter." @default.
• W2118601380 created "2016-06-24" @default.
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• W2118601380 date "2011-01-06" @default.
• W2118601380 modified "2023-10-16" @default.
• W2118601380 title "HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion" @default.
• W2118601380 cites W1819679722 @default.
• W2118601380 cites W1969750040 @default.
• W2118601380 cites W1978193295 @default.
• W2118601380 cites W1980744319 @default.
• W2118601380 cites W1982330083 @default.
• W2118601380 cites W1983027451 @default.
• W2118601380 cites W1983844641 @default.
• W2118601380 cites W1987922502 @default.
• W2118601380 cites W1988410625 @default.
• W2118601380 cites W1990523382 @default.
• W2118601380 cites W1992074382 @default.
• W2118601380 cites W1993011209 @default.
• W2118601380 cites W1995856471 @default.
• W2118601380 cites W1997235862 @default.
• W2118601380 cites W2005485346 @default.
• W2118601380 cites W2008687235 @default.
• W2118601380 cites W2010171257 @default.
• W2118601380 cites W2018196121 @default.
• W2118601380 cites W2022935142 @default.
• W2118601380 cites W2025965474 @default.
• W2118601380 cites W2030083850 @default.
• W2118601380 cites W2030605651 @default.
• W2118601380 cites W2032627363 @default.
• W2118601380 cites W2034255160 @default.
• W2118601380 cites W2037477551 @default.
• W2118601380 cites W2047170523 @default.
• W2118601380 cites W2048873715 @default.
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• W2118601380 cites W2051671594 @default.
• W2118601380 cites W2058569864 @default.
• W2118601380 cites W2062800307 @default.
• W2118601380 cites W2066256158 @default.
• W2118601380 cites W2068618869 @default.
• W2118601380 cites W2069786714 @default.
• W2118601380 cites W2077005128 @default.
• W2118601380 cites W2082709748 @default.
• W2118601380 cites W2083671513 @default.
• W2118601380 cites W2085061516 @default.
• W2118601380 cites W2089739884 @default.
• W2118601380 cites W2092404324 @default.
• W2118601380 cites W2097088124 @default.
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• W2118601380 cites W3100880512 @default.
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• W2118601380 doi "https://doi.org/10.1051/0004-6361/201015830" @default.
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