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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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發(fā)表于 2025-3-25 05:07:20 | 只看該作者
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發(fā)表于 2025-3-25 08:26:35 | 只看該作者
,Towards Constraining Tidal Mixing: U?Gru,em U?Gru. We build upon the initial findings of (Bowman et?al. .) with orbital phase-resolved spectroscopy of U?Gru obtained with UVES via ESO Directors Discretionary Time. We review the data of the system, perform spectroscopic disentangling, determine the orbital and atmospheric parameters, and in
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發(fā)表于 2025-3-25 15:33:50 | 只看該作者
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發(fā)表于 2025-3-25 18:39:15 | 只看該作者
2190-5053 a robust statistical framework to account for correlations, this methodology is employed to analyse individual stars, multiple systems, and clusters alike to demonstrate that chemical mixing has dramatic impact on stellar structure and evolution.978-3-030-66312-4978-3-030-66310-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
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發(fā)表于 2025-3-25 22:52:56 | 只看該作者
sses. Furthermore, the proposed framework generates appropriate Java code for integrating countermeasures, attacks, and smart vehicle models. To demonstrate the effectiveness of the proposed solution, we model, analyze, harden, and evaluate our framework using a real-world use case. This research ai
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發(fā)表于 2025-3-26 01:22:37 | 只看該作者
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發(fā)表于 2025-3-26 04:33:39 | 只看該作者
Cole Johnstonnsor node in the WSN is equipped with an LA so that it can autonomously select its proper state, i.e., either sleep or active with the aim to cover all targets with the lowest energy cost. Through comprehensive experimental testing, we verify the efficiency of our algorithm and its ability to yield
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發(fā)表于 2025-3-26 10:13:08 | 只看該作者
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