关于 Maia 星脉动可能解释的探讨
太阳与恒星天体物理
2017-11-08 v1
摘要
对若干年轻疏散星团的长期测光巡天，使我们得以识别出位于 HR 图上明确定义的 Scuti 变星与慢脉动 B 型星之间的恒星的光变现象。通过对 Kepler 数据的分析，也提出了若干此类天体。假设这种光变性源于脉动，我们试图用涉及自转和/或平均不透明度廓线修改的脉动模型来解释观测到的频率。
引用
@article{arxiv.1701.00937,
title = {On possible explanations of pulsations in Maia stars},
author = {Jadwiga Daszynska-Daszkiewicz and Przemyslaw Walczak and Alexey Pamyatnykh},
journal= {arXiv preprint arXiv:1701.00937},
year = {2017}
}
备注
proceedings of the Joint TASC2 - KASC9 Workshop - SPACEINN - HELAS8 Conference "Seismology of the Sun and the Distant Stars 2016", to be published by the EPJ Web of Conferences