Titlebook: Disks and Outflows Around Young Stars; Proceedings of a Con Steven Beckwith,Jakob Staude,Antonella Natta Conference proceedings 1996 Spring

BRIDE

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

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Seminar

978-3-662-15720-6Springer-Verlag Berlin Heidelberg 1996

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Lecture Notes in Physicshttp://image.papertrans.cn/e/image/281394.jpg

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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

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

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Parabola

人类学家

Keplerian circumstellar disks in Taurus: The GG Tau Ring and the DM Tau Disk,

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