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CO (2–1) observations of Maffei 2

Sargent, Anneila I. and Sutton, E. C. and Masson, C. R. and Phillips, T. G. and Lo, K.-Y. (1985) CO (2–1) observations of Maffei 2. In: The Milky Way Galaxy. IAU Symposium Proceedings Series. No.106. D. Reidel , Dordrecht, pp. 197-198. ISBN 9789400952911. https://resolver.caltech.edu/CaltechAUTHORS:20181211-154717976

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Abstract

Maffei 2 is a highly obscured galaxy, probably of type Sbc, at a distance of 5 Mpc (Allen and Raimond 1972; Spinrad et al. 1973). Since it lies close to the Galactic plane, there is considerable confusion in infrared and 21-cm HI observations due to Galactic emission, but investigations of its structure can be carried out at millimeter wavelengths where the Galaxy contribution is confined to a limited velocity range. The high resolution (30″) of our CO J=2–1 observations permits both a detailed examination of Maffei 2 and a study of the nature of the gas in its nucleus, through comparison with the CO J=1–0 observations.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1017/S0074180900242411DOIArticle
ORCID:
AuthorORCID
Sargent, Anneila I.0000-0002-4633-5098
Additional Information:© 1985 by the IAU.
Series Name:IAU Symposium Proceedings Series
Issue or Number:106
Record Number:CaltechAUTHORS:20181211-154717976
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20181211-154717976
Official Citation:Sargent, A., Sutton, E., Masson, C., Phillips, T., & Lo, K. (1985). CO (2–1) observations of Maffei 2. Symposium - International Astronomical Union, 106, 197-198. doi:10.1017/S0074180900242411
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:91696
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:11 Dec 2018 23:57
Last Modified:03 Oct 2019 20:37

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