Fluctuate
发表于 2025-3-28 17:53:35
Monte-Carlo Simulation as a Defining Tool to Diagnose Timing and Spectral Properties of Flows Aroundm is a classic example where Monte-Carlo simulation has been found to be very useful. This Chapter deals with the schematics that have been utilized. Spectral variations with various parameters are shown.
巨大没有
发表于 2025-3-28 19:12:06
Conference proceedings 2018 contributions by about fifty scientists who work on diverse topics in contemporary astrophysics and space science including new and low-cost balloon borne experiments, planetary science, astrochemistry and the origin of life, ionospheric research and earthquake predictions, relativistic astrophysic
易碎
发表于 2025-3-29 00:31:20
http://reply.papertrans.cn/32/3197/319680/319680_43.png
粘连
发表于 2025-3-29 05:15:57
http://reply.papertrans.cn/32/3197/319680/319680_44.png
打谷工具
发表于 2025-3-29 11:14:59
http://reply.papertrans.cn/32/3197/319680/319680_45.png
Commemorate
发表于 2025-3-29 11:24:12
http://reply.papertrans.cn/32/3197/319680/319680_46.png
Femish
发表于 2025-3-29 17:17:29
https://doi.org/10.1007/978-94-011-0111-0y to study simultaneously the time dependence of the disk structure and its spectral as well as temporal properties. We prove several of the conjectures that were made earlier based on theoretical studies and other simulations. We also discuss the current developments in this simulation code and the future scopes.
宴会
发表于 2025-3-29 23:36:07
http://reply.papertrans.cn/32/3197/319680/319680_48.png
OUTRE
发表于 2025-3-30 03:19:34
Evolution of Imaging of Black Hole Accretion-Outflow System over Half a Centuryof this century. Event Horizon Telescope (EHT) is getting prepared to discern the horizon of Sgr A* where radio interferometry technique has been deployed. For Galactic black holes, the required resolution is much higher and X-ray interferometry is essential.
身心疲惫
发表于 2025-3-30 06:15:54
On the Nature of Outflows from Low Angular Momentum Inflows Around Black Holespported shock wave in case of low angular momentum flow around black holes may be responsible for jets and outflows. The energy dissipation as well as mass loss rate across the shock may happen at the base of the jets and outflows. The outflow properties are determined by these parameters close to the black hole.