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• W3103251146 endingPage "543" @default.
• W3103251146 startingPage "525" @default.
• W3103251146 abstract "We present an analysis of LMXBs and GCs in five early-type galaxies using Chandra X-ray and HST optical data. Of the 186 LMXBs within the optical fields of view, 71 are in GCs, confirming that LMXBs are formed particularly efficiently in clusters due to dynamical interactions. However, there is no statistically significant correlation between the distance of a cluster from the center of its host galaxy and its LMXB hosting probability. LMXBs are preferentially found in luminous and metal-rich GCs. Metal-rich clusters are 3.4 times more likely to host LMXBs than metal-poor ones. This is slightly higher than that measured in other surveys, likely because of larger contamination of the GC sample in previous ground-based data sets and the inclusion of galaxies with intermediate-age clusters in others. Intriguingly, the LMXBs in NGC 1399 are preferentially in the reddest clusters of the metal-rich GC subsystem. This indicates that the red peak of the bimodal GC color distribution itself encompasses clusters with a range of enrichment histories. The strength of this effect varies from galaxy to galaxy, possibly indicating differences in their metal enrichment histories. Field LMXBs in our program galaxies are more concentrated toward the center of their host galaxies than GC LMXBs. This suggests that a majority of field LMXBs are formed in situ and are not a population that has escaped from current GCs. This is consistent with previous specific frequency-based studies. The brightest X-ray sources in GCs appear to be preferentially associated with luminous, metal-rich clusters. We show that it is probable that some of these clusters host multiple bright LMXBs, while the probability is much lower for metal-poor GCs. If this interpretation is correct, our study implies that LMXBs in more metal-rich cluster systems should reveal a longer high-luminosity X-ray tail and show less X-ray variability than metal-poor cluster populations." @default.
• W3103251146 created "2020-11-23" @default.
• W3103251146 creator A5014143820 @default.
• W3103251146 creator A5023447906 @default.
• W3103251146 creator A5032859478 @default.
• W3103251146 date "2007-06-10" @default.
• W3103251146 modified "2023-09-27" @default.
• W3103251146 title "Probing the Formation of Low‐Mass X‐Ray Binaries in Globular Clusters and the Field" @default.
• W3103251146 cites W1542975304 @default.
• W3103251146 cites W1635505342 @default.
• W3103251146 cites W1679305370 @default.
• W3103251146 cites W1964561298 @default.
• W3103251146 cites W1969355557 @default.
• W3103251146 cites W1969358747 @default.
• W3103251146 cites W1970333333 @default.
• W3103251146 cites W1977217170 @default.
• W3103251146 cites W1979579042 @default.
• W3103251146 cites W1979733958 @default.
• W3103251146 cites W1980118658 @default.
• W3103251146 cites W1985192680 @default.
• W3103251146 cites W1985555736 @default.
• W3103251146 cites W1987645840 @default.
• W3103251146 cites W1990779755 @default.
• W3103251146 cites W1991463099 @default.
• W3103251146 cites W1994668948 @default.
• W3103251146 cites W1994671833 @default.
• W3103251146 cites W1995033962 @default.
• W3103251146 cites W1999844453 @default.
• W3103251146 cites W2006396245 @default.
• W3103251146 cites W2011022699 @default.
• W3103251146 cites W2012226958 @default.
• W3103251146 cites W2013788304 @default.
• W3103251146 cites W2019928553 @default.
• W3103251146 cites W2020387858 @default.
• W3103251146 cites W2022005637 @default.
• W3103251146 cites W2024234951 @default.
• W3103251146 cites W2027765267 @default.
• W3103251146 cites W2031334387 @default.
• W3103251146 cites W2032166844 @default.
• W3103251146 cites W2033427105 @default.
• W3103251146 cites W2034754483 @default.
• W3103251146 cites W2053488603 @default.
• W3103251146 cites W2054363573 @default.
• W3103251146 cites W2054829847 @default.
• W3103251146 cites W2057847605 @default.
• W3103251146 cites W2063212296 @default.
• W3103251146 cites W2069147259 @default.
• W3103251146 cites W2069557347 @default.
• W3103251146 cites W2070451726 @default.
• W3103251146 cites W2073390875 @default.
• W3103251146 cites W2077232535 @default.
• W3103251146 cites W2088412696 @default.
• W3103251146 cites W2092904906 @default.
• W3103251146 cites W2094142432 @default.
• W3103251146 cites W2095078501 @default.
• W3103251146 cites W2110831150 @default.
• W3103251146 cites W2113154359 @default.
• W3103251146 cites W2114813636 @default.
• W3103251146 cites W2135884999 @default.
• W3103251146 cites W2138603295 @default.
• W3103251146 cites W2145110440 @default.
• W3103251146 cites W2145591315 @default.
• W3103251146 cites W2149639672 @default.
• W3103251146 cites W2157286649 @default.
• W3103251146 cites W2159248790 @default.
• W3103251146 cites W2951033192 @default.
• W3103251146 cites W3098109397 @default.
• W3103251146 cites W3099469848 @default.
• W3103251146 cites W3099801582 @default.
• W3103251146 cites W3100194952 @default.
• W3103251146 cites W3101075783 @default.
• W3103251146 cites W3101408682 @default.
• W3103251146 cites W3102202148 @default.
• W3103251146 cites W3102411808 @default.
• W3103251146 cites W3102945995 @default.
• W3103251146 cites W3103064439 @default.
• W3103251146 cites W3103368470 @default.
• W3103251146 cites W3103717250 @default.
• W3103251146 cites W3103829656 @default.
• W3103251146 cites W3104442489 @default.
• W3103251146 cites W3105443329 @default.
• W3103251146 cites W3105503988 @default.
• W3103251146 cites W3106221182 @default.
• W3103251146 cites W3106384588 @default.
• W3103251146 cites W3121595716 @default.
• W3103251146 cites W3121870099 @default.
• W3103251146 cites W3125341018 @default.
• W3103251146 cites W4229934221 @default.
• W3103251146 cites W4230259445 @default.
• W3103251146 cites W4241954951 @default.
• W3103251146 cites W4292480926 @default.
• W3103251146 cites W4299796995 @default.
• W3103251146 doi "https://doi.org/10.1086/518021" @default.
• W3103251146 hasPublicationYear "2007" @default.
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