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NASA NTRS · 20210003172

Disk Dispersal Around Young Stars

Abstract

We review the evidence pertaining to the lifetimes of planet-forming disks and discuss possible disk dispersal mechanisms: 1) viscous accretion of material onto the central source, 2) close stellar encounters, 3) stellar winds, and 4) photoevaporation by ultraviolet radiation.

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BibTeXRIS

Johnstone, D., Hollenbach, D., Yorke, H.. 1998-07-05. Disk Dispersal Around Young Stars. https://ntrs.nasa.gov/citations/20210003172

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