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- W3100616775 abstract "We have derived Mn abundances for more than 200 stars in 19 globular clusters. In addition, Mn abundance determinations have been made for a comparable number of halo field and disk stars possessing an overlapping range of metallicities and stellar parameters. Our primary data set was comprised of high-resolution spectra previously acquired at the McDonald, Lick, and Keck Observatories. To enlarge our data pool, we acquired globular and open cluster spectra from several other investigators. Data were analyzed using synthetic spectra of the 6000 Å Mn I triplet. Hyperfine structure parameters were included in the synthetic spectra computations. Our analysis shows that for the metallicity range -0.7 > [Fe/H] > -2.7, stars of 19 globular clusters have a mean relative abundance of = -0.37 ± 0.01 (σ = 0.10), a value in agreement with that of the field stars, = -0.36 ± 0.01 (σ = 0.08). Despite the 2 orders of magnitude span in metallicity, the ⟨[Mn/Fe]⟩ ratio remains constant in both stellar populations. Our Mn abundance data indicate that there is no appreciable variation in the relative nucleosynthetic contribution from massive stars that undergo core-collapse supernovae and thus no significant change of the associated initial mass function in the specified metallicity range." @default.
- W3100616775 created "2020-11-23" @default.
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- W3100616775 date "2006-06-01" @default.
- W3100616775 modified "2023-10-01" @default.
- W3100616775 title "Manganese Abundances in Cluster and Field Stars" @default.
- W3100616775 cites W1964118876 @default.
- W3100616775 cites W1965561594 @default.
- W3100616775 cites W1966724690 @default.
- W3100616775 cites W1967911932 @default.
- W3100616775 cites W1975114210 @default.
- W3100616775 cites W1976646714 @default.
- W3100616775 cites W1977457396 @default.
- W3100616775 cites W1979183860 @default.
- W3100616775 cites W1981504089 @default.
- W3100616775 cites W1982229516 @default.
- W3100616775 cites W1982661198 @default.
- W3100616775 cites W1987861871 @default.
- W3100616775 cites W1988090704 @default.
- W3100616775 cites W1991353966 @default.
- W3100616775 cites W1996891172 @default.
- W3100616775 cites W1998001053 @default.
- W3100616775 cites W1999277926 @default.
- W3100616775 cites W2000762108 @default.
- W3100616775 cites W2007124167 @default.
- W3100616775 cites W2007200000 @default.
- W3100616775 cites W2009195198 @default.
- W3100616775 cites W2011478974 @default.
- W3100616775 cites W2013962707 @default.
- W3100616775 cites W2016268550 @default.
- W3100616775 cites W2020836593 @default.
- W3100616775 cites W2021860039 @default.
- W3100616775 cites W2022330560 @default.
- W3100616775 cites W2024571432 @default.
- W3100616775 cites W2029384527 @default.
- W3100616775 cites W2032515733 @default.
- W3100616775 cites W2032927073 @default.
- W3100616775 cites W2047798125 @default.
- W3100616775 cites W2048596341 @default.
- W3100616775 cites W2050574667 @default.
- W3100616775 cites W2050790396 @default.
- W3100616775 cites W2052619536 @default.
- W3100616775 cites W2052805228 @default.
- W3100616775 cites W2059519221 @default.
- W3100616775 cites W2060195076 @default.
- W3100616775 cites W2064514344 @default.
- W3100616775 cites W2068241295 @default.
- W3100616775 cites W2071745231 @default.
- W3100616775 cites W2072957218 @default.
- W3100616775 cites W2096471541 @default.
- W3100616775 cites W2103024508 @default.
- W3100616775 cites W2103367868 @default.
- W3100616775 cites W2106648118 @default.
- W3100616775 cites W2110253451 @default.
- W3100616775 cites W2121463223 @default.
- W3100616775 cites W2126331421 @default.
- W3100616775 cites W2133437999 @default.
- W3100616775 cites W2149919814 @default.
- W3100616775 cites W2151302933 @default.
- W3100616775 cites W2157594202 @default.
- W3100616775 cites W2159752461 @default.
- W3100616775 cites W2171734876 @default.
- W3100616775 cites W2342062453 @default.
- W3100616775 cites W3048052109 @default.
- W3100616775 cites W3099500220 @default.
- W3100616775 cites W3099819036 @default.
- W3100616775 cites W3101076332 @default.
- W3100616775 cites W3101923103 @default.
- W3100616775 cites W3102189571 @default.
- W3100616775 cites W3103168846 @default.
- W3100616775 cites W3104832054 @default.
- W3100616775 cites W3105777284 @default.
- W3100616775 cites W3121389110 @default.
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- W3100616775 doi "https://doi.org/10.1086/503106" @default.
- W3100616775 hasPublicationYear "2006" @default.
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