arousal 发表于 2025-3-23 11:53:02
Course 2: 2D Transonic Hydrodynamics in General Relativity,978-1-349-81550-0细菌等 发表于 2025-3-23 17:16:06
http://reply.papertrans.cn/15/1438/143799/143799_12.pngAMOR 发表于 2025-3-23 18:11:31
Course 7: Cosmic Rays and Particle Acceleration at Astrophysical Shocks,978-3-030-63868-9GRAVE 发表于 2025-3-24 01:49:19
Course 9: Accretion around Active Galactic Nuclei,978-3-211-47311-5Congregate 发表于 2025-3-24 05:20:54
Accretion Disks, Jets and High-Energy Phenomena in AstrophysicsLes Houches SessionInnovative 发表于 2025-3-24 09:17:20
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http://reply.papertrans.cn/15/1438/143799/143799_17.pngB-cell 发表于 2025-3-24 15:09:42
Inflammatory Diseases Affecting Melanocytesion of a few key observationnal facts that lead to a threestep theoretical scenario. The physical processes at work in each step are then presented, focussing on the internal/external shock model. The last part briefly mention the possible non-photonic emission of gamma-ray bursts.palette 发表于 2025-3-24 20:43:16
http://reply.papertrans.cn/15/1438/143799/143799_19.pngCulpable 发表于 2025-3-24 23:23:00
Cutaneous Bacterial Infections,mstellar disks. In this review, we examine if, and how, the ubiquitous X-ray emission from young stars, taken as a proxy for magnetic reconnection events, can constrain the “central engine”, ., the magnetic structures widely thought to couple accretion and ejection.