沉积物 发表于 2025-3-25 05:33:06
http://reply.papertrans.cn/51/5009/500880/500880_21.pngChronic 发表于 2025-3-25 08:32:54
José Gracia,Fabio Colle,Turlough DownesProvides an introduction to modern high-performance computational methods.Reviews state-of-the-art results on jet and star formation.Includes supplementary material:Deadpan 发表于 2025-3-25 15:44:37
Lecture Notes in Physicshttp://image.papertrans.cn/j/image/500880.jpgarthroscopy 发表于 2025-3-25 17:57:10
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Modeling Accretion and Ejection Phenomena Around Young Stars: A Numerical PerspectiveThis chapter presents an overview of models based on time-dependent numerical simulations of the central regions of accreting T Tauri stars. The focus is put on magnetohydrodynamical studies of the launching mechanism of T Tauri jets (disk–winds, stellar winds, magnetospheric ejections) and of the magnetic star–disk interaction.Adulterate 发表于 2025-3-26 09:47:19
PK parameters derived for these binaries are again in full agreement with general relativity. Timing analysis of other pulsars contributes to very tight limits on other PPN parameters. Finally, we discuss how the Pulsar Timing Array can provide an effective tool to search for gravitational waves in印第安人 发表于 2025-3-26 14:20:55
PK parameters derived for these binaries are again in full agreement with general relativity. Timing analysis of other pulsars contributes to very tight limits on other PPN parameters. Finally, we discuss how the Pulsar Timing Array can provide an effective tool to search for gravitational waves in偶像 发表于 2025-3-26 18:15:32
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