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Inverse Correlation of the Ratios of S-Element Abundances in AGB Stars with Metallicity |
| ZHANG Bo;LIU Jun-hong;LIANG Yan-chun;PENG Qiu-he |
| 1Department of Physics, Hebei Normal University, Shijiazhuang 050016
2Department of Physics, Shijiazhuang Teachers College, Shijiazhuang 050041
3Department of Astronomy, Nanjing University, Nanjing, 210093
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| Cite this article: |
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ZHANG Bo, LIU Jun-hong, LIANG Yan-chun et al 1998 Chin. Phys. Lett. 15 76-78 |
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Abstract In present study, the relations between the ratios of the heavy to light s-element (slow neutron captrue element) abundances and the average neutron exposure are calculated for the intrinsic and extrinsic AGB stars, respectively. In addition, the inverse correlation of these ratios with metallicity is also presented and interpreted quantitatively. This work is based on the evolution of the heavy element abundances of the intrinsic AGB stars, and the calculation on the heavy element overabundances of the extrinsic AGB stars.
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| Keywords:
97.30.Hk
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Published: 01 January 1998
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| PACS: |
97.30.Hk
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(Carbon stars, S stars, and related types (C, S, R, and N))
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