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Disk Dispersal Around Young StarsWe 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.
Document ID
20210003172
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
hdl:2014/16902
Authors
Johnstone, D.
Hollenbach, D.
Yorke, H.
Date Acquired
July 5, 1998
Publication Date
July 5, 1998
Publication Information
Publisher: UNKNOWN
Distribution Limits
Public
Copyright
Other
Technical Review
Keywords
circumstellar
disks
ISM
circumstellar
matter
protoplanetary
disks
star
formation
planet
formation
HII
regions

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