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Titlebook: Interior Modelling of Massive Stars in Multiple Systems; Cole Johnston Book 2021 The Editor(s) (if applicable) and The Author(s), under ex

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樓主: Disaster
31#
發(fā)表于 2025-3-26 23:15:07 | 只看該作者
32#
發(fā)表于 2025-3-27 03:31:25 | 只看該作者
Cole Johnstonf the conditions of the patients. The platform will also help Healthcare providers to interact with medical history records. Furthermore, we propose an intelligent agent to release the doctors from requesting updates about historical records and to help doctors in diagnosing disease. We run simulati
33#
發(fā)表于 2025-3-27 05:32:59 | 只看該作者
Cole Johnstonaches to detect DDoS and discuss their strengths and weaknesses. Besides, we compare the existing methods based on their accuracy rate. Finally, we give an insight of future directions for DDoS detection in the SDN environment using the presented approaches.
34#
發(fā)表于 2025-3-27 10:39:28 | 只看該作者
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發(fā)表于 2025-3-27 14:20:21 | 只看該作者
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發(fā)表于 2025-3-27 20:37:06 | 只看該作者
2190-5053 ings of young massive stars.Includes a self-contained descriThis thesis by Cole Johnston brings novel insights into the inner workings of young massive stars. By bridging the observational fields of binary stars and asteroseismology this thesis uses state of the art statistical techniques to scrutin
37#
發(fā)表于 2025-3-28 02:00:40 | 只看該作者
Book 2021s and asteroseismology this thesis uses state of the art statistical techniques to scrutinise? theories of modern stellar astrophysics. Developing upon the commonly used isochrone fitting methodology, the author introduces the idea of isochrone cloud fitting in order to account for the full breadth
38#
發(fā)表于 2025-3-28 06:09:20 | 只看該作者
Scientific Context,ulsating stars as well as binary stars and clusters. We conclude by summarising the current state-of-the-art and how studying pulsating stars and stars in multiple systems reveal shortcomings in the theory of stellar structure and evolution.
39#
發(fā)表于 2025-3-28 09:00:06 | 只看該作者
40#
發(fā)表于 2025-3-28 13:13:32 | 只看該作者
The O+B Eclipsing Binary HD 165246, variability observed in the massive O+B eclipsing binary HD?165246. We make use of space-based photometry assembled with the .2 mission as well as ground-based spectroscopy to characterise the pulsational variability observed in HD?165246.
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