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 | ||||||
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Additional Information: | © 1985 by the IAU. | ||||||
Series Name: | IAU Symposium Proceedings Series | ||||||
Issue or Number: | 106 | ||||||
DOI: | 10.1017/S0074180900242411 | ||||||
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: | 16 Nov 2021 03:43 |
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