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The evolution of protostellar disks under the influence of external UV radiation and central stellar windsThe evolution and appearance of circumstellar disks in star forming regions can be influenced strongly by the radiation from nearby hot stars. Here we describe the results of numerical simulations of the evolution of protostellar disks and their immediate surroundings under the influence of external UV radiation.
Document ID
20060031034
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Yorke, H. W.
Richling, S.
Date Acquired
August 23, 2013
Publication Date
January 8, 2001
Distribution Limits
Public
Copyright
Other
Keywords
star formations circumstellar matter HII regions

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