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Titlebook: Investigating the A-Type Stars Using Kepler Data; Simon J. Murphy Book 2015 Springer International Publishing Switzerland 2015 Asteroseism

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樓主: VEER
11#
發(fā)表于 2025-3-23 11:22:00 | 只看該作者
12#
發(fā)表于 2025-3-23 14:15:00 | 只看該作者
A Selective Review of Spectral Peculiarities in the A Stars,se and the Ap stars. Additionally, the two main theories for the origin of abundance anomalies in .?Boo stars are discussed and it is suggested that both of them imply the .?Boo stars contain a high fraction of pulsators—a suggestion that is backed up by observations in the literature.
13#
發(fā)表于 2025-3-23 20:47:02 | 只看該作者
https://doi.org/10.1007/978-3-319-09417-5Asteroseismology of A Stars; Chemically Peculiar Stars; Data Analysis of Kepler Data; Rotation of Stars
14#
發(fā)表于 2025-3-24 02:07:52 | 只看該作者
978-3-319-36323-3Springer International Publishing Switzerland 2015
15#
發(fā)表于 2025-3-24 04:04:39 | 只看該作者
Investigating the A-Type Stars Using Kepler Data978-3-319-09417-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
16#
發(fā)表于 2025-3-24 10:02:10 | 只看該作者
Conclusions and Future Work,This chapter focusses on the main conclusions of the thesis and the future prospects thereof. More detailed conclusions can be found at the end of each chapter.
17#
發(fā)表于 2025-3-24 12:07:36 | 只看該作者
18#
發(fā)表于 2025-3-24 18:21:07 | 只看該作者
Springer Theseshttp://image.papertrans.cn/i/image/474769.jpg
19#
發(fā)表于 2025-3-24 20:15:26 | 只看該作者
, Catalogues and Published Case Studies,e case studies are presented as published, and are stand-alone journal articles, but are additionally contextualised by the review of the literature on pulsating stars that was presented in the previous chapter. Also described and presented are catalogues of . data that I have used to select stars for case studies.
20#
發(fā)表于 2025-3-25 00:47:24 | 只看該作者
2190-5053 hree decades.Demonstrates novel techniques for asteroseismolSimon Murphy‘s thesis has significant impact on the wide use of the revolutionary Kepler Mission data, leading to a new understanding in stellar astrophysics.?It first provides a deep characterisation and comparison of the Kepler long caden
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