Binary post-AGB stars

被引：0

作者：

Van Winckel, H ^{[1
]}

Maas, T ^{[1
]}

Lloyd-Evans, T ^{[1
]}

机构：

[1] Katholieke Univ Leuven, Inst Sterrenkunde, B-3001 Louvain, Heverlee, Belgium

来源：

ASYMMETRICAL PLANETARY NEBULAE III | 2004年 / 313卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report here on our ongoing systematic radial velocity monitoring programme of a sample of post-AGB stars. The programme stars are evolved objects with SED characteristics indicative of a dusty disc. The sample was originally tuned to discover new RV Tauri stars (G-K supergiants showing stellar pulsations with alternating deep and shallow minima) by Lloyd Evans (1999). We confirm the suspected high binary fraction.

引用

页码：536 / 537

页数：2

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