主序星脉动模式的识别：潜力与局限
太阳与恒星天体物理
2011-12-13 v1
摘要
我们回顾了应用于主序脉动星的模式识别方法，重点聚焦于利用多色测光和径向速度数据的方法。讨论了可能影响这些观测量诊断特性的效应。我们还提出了高角阶模式识别的问题，此类模式在基于空间项目的观测谱中可能占据主导地位。
引用
@article{arxiv.1112.2572,
title = {Identification of Pulsation Modes in Main Sequence Stars: Potentials and Limits},
author = {J. Daszyńska-Daszkiewicz and A. A. Pamyatnykh},
journal= {arXiv preprint arXiv:1112.2572},
year = {2011}
}
备注
6 pages, 4 figures, invited talk at the 20th Stellar Pulsation Conference "Impact of new instrumentation and new insights in stellar pulsations" (5-9 September 2011, Granada, Spain). Astrophys. Space Sci. Proc. series (ASSP), eds. L. Balona, J. Christensen-Dalsgaard, R. Garrido and J. C. Suarez (in press)