BRIDE
发表于 2025-3-26 21:40:30
Physical processes in circumstellar disks,h disk accretion and secondary bodies within the disk. Next, we consider the viscous evolution of disks and the possible sources of the viscosity. We briefly consider magnetic instabilities tidal effects, and vortex motions. We also discuss the process of planet formation
assent
发表于 2025-3-27 02:58:14
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Seminar
发表于 2025-3-27 07:04:33
978-3-662-15720-6Springer-Verlag Berlin Heidelberg 1996
爱得痛了
发表于 2025-3-27 11:36:16
Lecture Notes in Physicshttp://image.papertrans.cn/e/image/281394.jpg
碌碌之人
发表于 2025-3-27 15:57:11
The FU orionis outburst as a thermal accretion event: Theoretical and observational implications,iscosity has implications for self gravity as a possible mass transport mechanism through much of the disk. Light curves of V1515 Cyg, FU Ori, and V1057 Cyg are reproduced, and model results are compared to observations.
诱惑
发表于 2025-3-27 18:00:08
The stellar populations of deeply embedded young clusters: Near-infrared spectral classification,sample covers a range of spectral types and disk accretion rates including classical and weak-lined T Tauri stars. Results suggest that spectral types derived from infrared spectra agree with their optically derived counterparts to within a few subclasses for late-type stars. Further, weak-lined T T
Exhilarate
发表于 2025-3-28 00:30:55
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Parabola
发表于 2025-3-28 05:40:16
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人类学家
发表于 2025-3-28 09:13:48
Keplerian circumstellar disks in Taurus: The GG Tau Ring and the DM Tau Disk,
大厅
发表于 2025-3-28 12:43:57
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