標(biāo)題: Titlebook: Interior Modelling of Massive Stars in Multiple Systems; Cole Johnston Book 2021 The Editor(s) (if applicable) and The Author(s), under ex [打印本頁(yè)] 作者: Disaster 時(shí)間: 2025-3-21 16:57
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書(shū)目名稱(chēng)Interior Modelling of Massive Stars in Multiple Systems讀者反饋學(xué)科排名
作者: chronicle 時(shí)間: 2025-3-21 21:04
Springer Theseshttp://image.papertrans.cn/i/image/471041.jpg作者: 受人支配 時(shí)間: 2025-3-22 01:19 作者: canvass 時(shí)間: 2025-3-22 05:13 作者: Rejuvenate 時(shí)間: 2025-3-22 12:24 作者: 越自我 時(shí)間: 2025-3-22 13:34 作者: 禁令 時(shí)間: 2025-3-22 19:46
Cole Johnston fields such as target coverage, battlefield surveillance, home security, health care supervision, and many more. However, power usage in WSNs remains a challenging issue due to the low capacity of batteries and the difficulty of replacing or charging them, especially in harsh environments. Therefor作者: FILLY 時(shí)間: 2025-3-22 23:26 作者: 轎車(chē) 時(shí)間: 2025-3-23 05:25 作者: cartilage 時(shí)間: 2025-3-23 06:13 作者: ALTER 時(shí)間: 2025-3-23 09:47 作者: 冷淡周邊 時(shí)間: 2025-3-23 15:20
Cole Johnstontwork administration, programmability, and elasticity. However, due to the centralized control method of SDN, threats to system vulnerabilities can damage the privacy, integrity, and confidentiality of the system, reducing network security, performance, and efficiency. Distributed Denial of Service 作者: conjunctivitis 時(shí)間: 2025-3-23 21:46
Cole Johnstoncal services at remote areas through an effective communication between healthcare providers. The healthcare stakeholders (including the doctors, nurses, etc.) are facing tremendous problems to track the conditions of the patients, trace them, and coordinate their interventions. In several cases, th作者: ATRIA 時(shí)間: 2025-3-24 02:04 作者: 存心 時(shí)間: 2025-3-24 03:24 作者: 難管 時(shí)間: 2025-3-24 06:34
Scientific Context,es. Then, we discuss the transport of chemicals within a star according to different types of mixing processes. Next, we discuss the course of stellar evolution first without considering chemical transport, and then with considering chemical transport and how it alters the stellar interior and the c作者: nutrients 時(shí)間: 2025-3-24 14:34 作者: FANG 時(shí)間: 2025-3-24 16:50
The O+B Eclipsing Binary HD 165246,ir evolution, including pulsations, chemical transport, wind mass-loss, rapid rotation, multiplicity, etc. In this chapter, we investigate the diverse 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 gr作者: Excise 時(shí)間: 2025-3-24 20:12 作者: EPT 時(shí)間: 2025-3-25 01:25
Binary Asteroseismology,ramework established in Chap.?. and the results of Chap.?., we now investigate to what extent the inclusion of complementary asteroseismic information augments our modelling procedure. We briefly introduce the topic and address the application of the statistical framework to our current modelling ef作者: COLON 時(shí)間: 2025-3-25 05:07 作者: intellect 時(shí)間: 2025-3-25 08:26
,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作者: exceptional 時(shí)間: 2025-3-25 15:33 作者: FORGO 時(shí)間: 2025-3-25 18:39
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 作者: EVEN 時(shí)間: 2025-3-25 22:52
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作者: homocysteine 時(shí)間: 2025-3-26 01:22 作者: Harbor 時(shí)間: 2025-3-26 04:33
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 作者: 財(cái)主 時(shí)間: 2025-3-26 10:13 作者: 膠水 時(shí)間: 2025-3-26 16:25 作者: 延期 時(shí)間: 2025-3-26 18:46 作者: affluent 時(shí)間: 2025-3-26 23:15 作者: Noctambulant 時(shí)間: 2025-3-27 03:31
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作者: promote 時(shí)間: 2025-3-27 05:32
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.作者: 終止 時(shí)間: 2025-3-27 10:39 作者: 啜泣 時(shí)間: 2025-3-27 14:20 作者: Fillet,Filet 時(shí)間: 2025-3-27 20:37
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作者: 衣服 時(shí)間: 2025-3-28 02:00
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 作者: 詞匯表 時(shí)間: 2025-3-28 06:09
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.作者: 拖網(wǎng) 時(shí)間: 2025-3-28 09:00 作者: 蒙太奇 時(shí)間: 2025-3-28 13:13
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.作者: sigmoid-colon 時(shí)間: 2025-3-28 17:36
