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Molecular Disks Around Young Stars

Published online by Cambridge University Press:  12 April 2016

Anneila I. Sargent  and
Steven V. W. Beckwith
Anneila I. Sargent
Affiliation:
California Institute of Technology, Pasadena, CA 91125
Steven V. W. Beckwith
Affiliation:
Cornell University, Ithaca, NY 14853

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There is now a substantial body of evidence that disk-like structures of gas and dust surround many protostars and young stellar objects (e.g. Rodriguez, these proceedings). We are currently studying a number of these disks to establish whether they have properties compatible with those attributed to the proto-solar nebula, in the early stages of evolution of our solar system. The frequency with which such proto-planetary disks are associated with young stars is also being investigated.

Type
III. Discs, Outflows, Jets and HH Objects
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 215 - 220
Copyright
Copyright © Springer-Verlag 1989

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