Asteroseismic data analysis: foundations and techniques
Asteroseismic data analysis: foundations and techniques
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星震数据分析：基础和技术
DOI：
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发表时间：
2019
期刊：
影响因子：
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通讯作者：
P. McClintock
中科院分区：
文献类型：
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作者：
P. McClintock
恒星是有脉动的，它们脉动的性质可以提供很多关于它们的信息，例如，它们的质量、半径和年龄。很久以前，在16世纪末，人们第一次观察到恒星亮度的波动。从那时起，人们已经确定这种现象似乎是恒星普遍存在的特征，对它的研究被命名为星震学。
Stars pulsate and their nature of their pulsations can provide a great deal of information about them including, for example, their masses, radii and ages. Oscillations in stellar brightness were first observed long ago, at the end of the sixteenth century. Since then, it has been established the phenomenon is seemingly a ubiquitous feature of stars and its study has been named asteroseismology.