BLUSH
发表于 2025-3-23 11:22:00
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hemoglobin
发表于 2025-3-23 14:15:00
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.
法律的瑕疵
发表于 2025-3-23 20:47:02
https://doi.org/10.1007/978-3-319-09417-5Asteroseismology of A Stars; Chemically Peculiar Stars; Data Analysis of Kepler Data; Rotation of Stars
微枝末节
发表于 2025-3-24 02:07:52
978-3-319-36323-3Springer International Publishing Switzerland 2015
镇痛剂
发表于 2025-3-24 04:04:39
Investigating the A-Type Stars Using Kepler Data978-3-319-09417-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
石墨
发表于 2025-3-24 10:02:10
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.
nullify
发表于 2025-3-24 12:07:36
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泛滥
发表于 2025-3-24 18:21:07
Springer Theseshttp://image.papertrans.cn/i/image/474769.jpg
表皮
发表于 2025-3-24 20:15:26
, 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.
赏钱
发表于 2025-3-25 00:47:24
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