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Molecular Gas in the Nucleus of M82

Lo, K. Y. and Cheung, K. W. and Masson, C. R. and Phillips, T. G. and Scoville, N. Z. and Woody, D. P. (1987) Molecular Gas in the Nucleus of M82. In: Star Forming Regions. IAU Symposium Proceedings Series. No.115. D. Reidel , Dordrecht, pp. 620-621. ISBN 9789027723888. https://resolver.caltech.edu/CaltechAUTHORS:20181116-103500590

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Abstract

7″-resolution CO (1-0) observations of M82 with the Owens Valley millimeter-wave interferometer have resolved 2 components of molecular gas in the central 1.5 arcmin of the galaxy: (1) a high plane of M82, and (2) shell-like or filamentary structures of molecular gas, with size-scale as large as 400 pc, extending most likely out of the plane of the galaxy.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1017/S0074180900096534DOIArticle
ORCID:
AuthorORCID
Scoville, N. Z.0000-0002-0438-3323
Additional Information:© 1987 Reidel.
Series Name:IAU Symposium Proceedings Series
Issue or Number:115
Record Number:CaltechAUTHORS:20181116-103500590
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20181116-103500590
Official Citation:Lo, K., Cheung, K., Masson, C., Phillips, T., Scoville, N., & Woody, D. (1987). Molecular Gas in the Nucleus of M82. Symposium - International Astronomical Union, 115, 620-621. doi:10.1017/S0074180900096534
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:90962
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:16 Nov 2018 18:46
Last Modified:03 Oct 2019 20:30

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