Observations versus theory:: The δ Scuti star CD-24 7599

被引：0
|
作者：
Pikall, H [1 ]
Handler, G [1 ]
Pamyatnykh, AA [1 ]
Dziembowski, W [1 ]
机构：
[1] Univ Vienna, Inst Astron, A-1180 Vienna, Austria
来源：
HALF CENTURY OF STELLAR PULSATION INTERPRETATIONS: A TRIBUTE TO ARTHUR N. COX | 1998年 / 135卷
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present preliminary results of our theoretical efforts to reproduce the observed frequency spectrum of the delta Scuti star CD-24 7599 = XX Pyx. An attempt to match the observed frequencies by an objective method resulted in several best fitting model sequences; We cannot yet reproduce the observed frequencies within the observational errors. This suggests that both definite mode identifications from observations as well as further refinements of our models are needed.
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页码：486 / 487
页数：2
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