1985
DOI: 10.1007/978-3-642-82234-6_8
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Redefining Clinical Research

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Cited by 3 publications
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“…With so many varieties of stars which exhibit clear signatures of enhancements of the s-process in their abundance patterns, it is not surprising that a great deal of effort has been expended by observational spectroscopists in analyzing the details of s-process nucleosynthesis in the heavy-element rich stars. A number of detailed abundance analyses have been conducted on the various heavy-element rich stars over the last 15 years and can be summarized as follows: for the barium giants we have Tomkin & Lambert (1983, 1986, Smith (1984), AGB star photospheres 71 Kovacs (1985), Smith & Lambert (1984), Malaney & Lambert (1988), , while the main-sequence Ba stars have been studied by Tomkin et al (1989) and North et al (1994). The CH giants have been studied by Vanture (1992aVanture ( , 1992b.…”
Section: Vv Smithmentioning
confidence: 99%
“…With so many varieties of stars which exhibit clear signatures of enhancements of the s-process in their abundance patterns, it is not surprising that a great deal of effort has been expended by observational spectroscopists in analyzing the details of s-process nucleosynthesis in the heavy-element rich stars. A number of detailed abundance analyses have been conducted on the various heavy-element rich stars over the last 15 years and can be summarized as follows: for the barium giants we have Tomkin & Lambert (1983, 1986, Smith (1984), AGB star photospheres 71 Kovacs (1985), Smith & Lambert (1984), Malaney & Lambert (1988), , while the main-sequence Ba stars have been studied by Tomkin et al (1989) and North et al (1994). The CH giants have been studied by Vanture (1992aVanture ( , 1992b.…”
Section: Vv Smithmentioning
confidence: 99%