Maximizer
发表于 2025-3-28 18:07:22
http://reply.papertrans.cn/51/5009/500886/500886_41.png
Respond
发表于 2025-3-28 21:48:28
http://reply.papertrans.cn/51/5009/500886/500886_42.png
浪费物质
发表于 2025-3-29 00:08:31
T.A. Gardiner,A. Frank,E.G. Blackman,S.V. Lebedev,J.P. Chittenden,D. Ampleford,S.N. Bland,A. Ciardi,
类型
发表于 2025-3-29 03:51:02
K. Tsinganos,N. Vlahakis,S. Bogovalov,C. Sauty,E. Trussoni,J.J.G. Lima
简洁
发表于 2025-3-29 09:24:38
The Structure of Young Stellar Jets and Winds Revealed By High Resolution λL.644μM Line Obseinig a broad line width. The HVC is located farther away from the origin and is more extended than the LVC. Our results suggest that the HVC is a well-collimated jet originating from the region close to the star, while the LVC is a widely-opened wind accelerated in the region near the inner edge of the accretion disk.
要素
发表于 2025-3-29 15:09:43
Photoionization of Cool Mhd Disk Windstar. However, it is difficult to foresee how temperatures as high as ∼ 5 x 10. can be reached unless a significant fraction of the X-rays radiation is produced by magnetic reconnection at the boundary between the stellar magnetosphere and the accretion disk.
值得尊敬
发表于 2025-3-29 15:43:42
http://reply.papertrans.cn/51/5009/500886/500886_47.png
推延
发表于 2025-3-29 21:28:30
Magnetic Star-Disk Interaction in Classical T Tauri Systemsa solar-mass central star, an accretion rate of 10..⊙/., and a viscosity parameter αss = 0.01, a field strength of 1 kG, measured at the poles on the surface of the star, was found insufficient for disk disruption.
Banister
发表于 2025-3-30 00:05:45
http://reply.papertrans.cn/51/5009/500886/500886_49.png
挑剔为人
发表于 2025-3-30 06:39:44
Hh 111 Stis Observations and Their Analysis Using Analytical and Numerical Modelsall bowshock within the jet beam. In this paper we present a long-slit spectrum of Herbig-Haro object HH 111 obtained with STIS and an interpretation of this observation in terms of an ejection velocity variability model.