The carbon Cepheid RT Trianguli Australis:: additional evidence of triple-α and CNO cycling

被引:8
作者
Wallerstein, G [1 ]
Matt, S [1 ]
Gonzalez, G [1 ]
机构
[1] Univ Washington, Dept Astron, Seattle, WA 98195 USA
关键词
stars : abundances; stars : chemically peculiar; stars : individual : RT TrA; stars : individual : U TrA; stars : Population II; Cepheids;
D O I
10.1046/j.1365-8711.2000.03064.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have used echelle spectra of resolving power 35 000 to derive chemical abundances and the C-12/C-13 ratio in the 1.9-d carbon Cepheid RT TrA and the Cepheid U TrA, employed as a comparison star. We confirm that RT TrA is very metal-rich with [Fe/H ] = +0.4. In addition, C and N are substantially in excess, and a small deficiency in O is present. We interpret these anomalies as resulting from the appearance on the stellar surface of material enriched in C-12 by the 3-alpha process, followed by CNO cycling to convert C-12 to C-13 and N-14. In addition, some O-16 has been processed to N-14. The partial processing of O-16 to N-14 indicates that substantial O-17 may be present. Proton capture seems to have enhanced Na-23 from the Ne isotopes.
引用
收藏
页码:414 / 422
页数:9
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