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Molecular Disks Around Young Stars

Sargent, Anneila I. and Beckwith, Steven V. W. (1989) Molecular Disks Around Young Stars. In: Structure and Dynamics of the Interstellar Medium. IAU Symposium Proceedings Series. No.120. Springer , Berlin, pp. 215-220. ISBN 9783540519560. https://resolver.caltech.edu/CaltechAUTHORS:20181121-090050084

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Abstract

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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1017/S0252921100023769DOIArticle
https://rdcu.be/b4cD8PublisherFree ReadCube access
ORCID:
AuthorORCID
Sargent, Anneila I.0000-0002-4633-5098
Additional Information:© 1989 Springer-Verlag.
Series Name:IAU Symposium Proceedings Series
Issue or Number:120
Record Number:CaltechAUTHORS:20181121-090050084
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20181121-090050084
Official Citation:Sargent, A., & Beckwith, S. (1989). Molecular Disks Around Young Stars. International Astronomical Union Colloquium, 120, 215-220. doi:10.1017/S0252921100023769
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:91127
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Nov 2018 17:18
Last Modified:15 May 2020 23:45

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