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Kinematics of Molecular Clouds Near the Galactic Center

Scoville, N. Z. (1972) Kinematics of Molecular Clouds Near the Galactic Center. Astrophysical Journal, 175 . L127-L132. ISSN 0004-637X. http://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
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/181000DOIArticle
http://adsabs.harvard.edu/abs/1972ApJ...175L.127SADSArticle
ORCID:
AuthorORCID
Scoville, N. Z.0000-0002-0438-3323
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.
Record Number:CaltechAUTHORS:20190329-141817211
Persistent URL:http://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:29 Mar 2019 21:39

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