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- W2749278364 abstract "We analyzed the high-resolution spectra of a large sample of AGB and RGB stars in the Galactic globular clusters (GCs) NGC 104, NGC 6121, and NGC 6809 obtained with FLAMES/GIRAFFE at ESO/VLT, and determined their Na abundances. This is the first time that the AGB stars in NGC 6809 are targeted. Moreover, we reanalyzed with the same method the data archive for NGC 6752. To investigate the dependence of AGB Na abundance dispersion on GC parameters, we compared the AGB [Na/H] distributions we obtained (including NGC 2808 presented in the first paper of this series) with literature data for four other GCs, i.e., a total of nine GCs, covering a wide range of GC parameters. We find that NGC 104 and NGC 6809 have comparable AGB and RGB Na abundance distributions revealed by the K-S test, while NGC 6121 shows a lack of very Na-rich AGB star. By analyzing all the nine GCs, the Na abundances and multiple populations of AGB stars show a complex picture. In some GCs, AGB stars have similar Na abundances and/or second-population fractions as their RGB counterparts, while some GCs do not have Na-rich second-population AGB star, and various cases exist between the two extremes. In addition, the fitted relations between fractions of AGB second population and GC global parameters show that AGB second-population fraction slightly anticorrelates with GC central concentration, while no robust dependency can be confirmed with other GC parameters. Current data roughly support the prediction of FRMS scenario. However, considering the weak observational and theoretical trends where scatter and exceptions exist, the fraction of second-population AGB stars can be affected by more than one or two factors, and may even be a result of stochasticity." @default.
- W2749278364 created "2017-08-31" @default.
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- W2749278364 date "2017-08-25" @default.
- W2749278364 modified "2023-09-30" @default.
- W2749278364 title "Sodium abundances of AGB and RGB stars in Galactic globular clusters II. Analysis and results of NGC 104, NGC 6121 and NGC 6809" @default.
- W2749278364 cites W1614678536 @default.
- W2749278364 cites W1770209262 @default.
- W2749278364 cites W1862756473 @default.
- W2749278364 cites W1901877775 @default.
- W2749278364 cites W1910315639 @default.
- W2749278364 cites W1916050026 @default.
- W2749278364 cites W1974370742 @default.
- W2749278364 cites W1979257798 @default.
- W2749278364 cites W1979719427 @default.
- W2749278364 cites W1981256345 @default.
- W2749278364 cites W2014992560 @default.
- W2749278364 cites W2019720374 @default.
- W2749278364 cites W2020568364 @default.
- W2749278364 cites W2023597317 @default.
- W2749278364 cites W2026835293 @default.
- W2749278364 cites W2030838397 @default.
- W2749278364 cites W2037904784 @default.
- W2749278364 cites W2045692013 @default.
- W2749278364 cites W2050790396 @default.
- W2749278364 cites W2056932217 @default.
- W2749278364 cites W2060003482 @default.
- W2749278364 cites W2066406099 @default.
- W2749278364 cites W2068155198 @default.
- W2749278364 cites W2069568975 @default.
- W2749278364 cites W2072276085 @default.
- W2749278364 cites W2072385866 @default.
- W2749278364 cites W2073315801 @default.
- W2749278364 cites W2081944412 @default.
- W2749278364 cites W2082337583 @default.
- W2749278364 cites W2096433368 @default.
- W2749278364 cites W2102155954 @default.
- W2749278364 cites W2105801537 @default.
- W2749278364 cites W2106493508 @default.
- W2749278364 cites W2106695319 @default.
- W2749278364 cites W2115153841 @default.
- W2749278364 cites W2115446991 @default.
- W2749278364 cites W2116940688 @default.
- W2749278364 cites W2121872350 @default.
- W2749278364 cites W2127491161 @default.
- W2749278364 cites W2131745971 @default.
- W2749278364 cites W2135785862 @default.
- W2749278364 cites W2138613133 @default.
- W2749278364 cites W2138742840 @default.
- W2749278364 cites W2141201519 @default.
- W2749278364 cites W2142219892 @default.
- W2749278364 cites W2142220522 @default.
- W2749278364 cites W2152437300 @default.
- W2749278364 cites W2153483400 @default.
- W2749278364 cites W2155155328 @default.
- W2749278364 cites W2158606005 @default.
- W2749278364 cites W2165745660 @default.
- W2749278364 cites W2167635287 @default.
- W2749278364 cites W2268382917 @default.
- W2749278364 cites W2276065491 @default.
- W2749278364 cites W2336089742 @default.
- W2749278364 cites W2566120013 @default.
- W2749278364 cites W2581494544 @default.
- W2749278364 cites W2623313604 @default.
- W2749278364 cites W2899497983 @default.
- W2749278364 cites W2918136281 @default.
- W2749278364 cites W2950699083 @default.
- W2749278364 cites W3098184523 @default.
- W2749278364 cites W3098976997 @default.
- W2749278364 cites W3099139600 @default.
- W2749278364 cites W3099635862 @default.
- W2749278364 cites W3099670565 @default.
- W2749278364 cites W3099840315 @default.
- W2749278364 cites W3100060146 @default.
- W2749278364 cites W3100928122 @default.
- W2749278364 cites W3101124902 @default.
- W2749278364 cites W3102077215 @default.
- W2749278364 cites W3102087735 @default.
- W2749278364 cites W3103043790 @default.
- W2749278364 cites W3103661582 @default.
- W2749278364 cites W3104067953 @default.
- W2749278364 cites W3104497004 @default.
- W2749278364 cites W3104521320 @default.
- W2749278364 cites W3104525630 @default.
- W2749278364 cites W3104585307 @default.
- W2749278364 cites W3104662322 @default.
- W2749278364 cites W3104852806 @default.
- W2749278364 cites W3104956757 @default.
- W2749278364 cites W3105107009 @default.
- W2749278364 cites W3121944230 @default.
- W2749278364 cites W3124609170 @default.
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