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1.0 mm Continuum Observations of Cool Southern Clouds

Published online by Cambridge University Press:  14 August 2015

D. Y. Gezari ,
L. Cheung ,
M. G. Hauser  and
J. A. Frogel
D. Y. Gezari
Affiliation:
Infrared and Radio Astronomy Branch (Code 693.2) NASA/Goddard Space Flight Center, Greenbelt, MD. 20771
L. Cheung
Affiliation:
Infrared and Radio Astronomy Branch (Code 693.2) NASA/Goddard Space Flight Center, Greenbelt, MD. 20771
M. G. Hauser
Affiliation:
Infrared and Radio Astronomy Branch (Code 693.2) NASA/Goddard Space Flight Center, Greenbelt, MD. 20771
J. A. Frogel
Affiliation:
Cerro Tololo Inter-American Observatory, La Serena, Chile

Extract

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High surface brightness 1.0 mm continuum emission has been mapped in nine southern hemisphere HII/molecular cloud complexes: NGC 6334, RCW 38, RCW 57, RCW 122, RCW 117, G333.6-0.2, G351.6-1.3, W 33 and W 33A. All of the sources are located in the inner part of the Galaxy near the galactic plane. This paper presents new 1.0 mm continuum mapping results with 65 arc sec resolution. A more detailed discussion of the observations is given by Cheung et al. (1978, 1979).

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 129 - 132
Copyright
Copyright © Reidel 1980 

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