Scoville, N. Z. (1972) Kinematics of Molecular Clouds Near the Galactic Center. Astrophysical Journal, 175 . L127-L132. ISSN 0004-637X. doi:10.1086/181000. https://resolver.caltech.edu/CaltechAUTHORS:20190329-141817211
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Abstract
A model is proposed in which most of the molecular clouds near the galactic center are situated in a radially moving ring of radius 250 pc.
| Item Type: | Article | |||||||||
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| Additional Information: | © 1972. The American Astronomical Society. Received 1972 April 27. I would particularly like to thank R. H. Sanders for many stimulating discussions on this work. | |||||||||
| DOI: | 10.1086/181000 | |||||||||
| Record Number: | CaltechAUTHORS:20190329-141817211 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20190329-141817211 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 94293 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | George Porter | |||||||||
| Deposited On: | 29 Mar 2019 21:39 | |||||||||
| Last Modified: | 16 Nov 2021 17:04 |
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