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A new 4m millimeter-wave telescope for a southern sky CO survey

Published online by Cambridge University Press:  19 July 2016

Y. Fukui ,
H. Ogawa ,
K. Kawabata ,
A. Mizuno  and
K. Sugitani
Y. Fukui
Affiliation:
Department of Astrophysics, Nagoya University, Nagoya 464-01, Japan
H. Ogawa
Affiliation:
Department of Astrophysics, Nagoya University, Nagoya 464-01, Japan
K. Kawabata
Affiliation:
Department of Astrophysics, Nagoya University, Nagoya 464-01, Japan
A. Mizuno
Affiliation:
Department of Astrophysics, Nagoya University, Nagoya 464-01, Japan
K. Sugitani
Affiliation:
College of General Education, Nagoya City University, Nagoya, Japan

Abstract

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We plan to install a new 4m radiotelescope in Australia to complete a sky survey of star-forming regions in the millimeter-wave CO(J=1-0, J-2-1) emission.

Information

Type
Large-Scale Structure and Kinematics
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 105 - 106
Copyright
Copyright © Kluwer 1991 

References

Ogawa, H., Mizuno, A., Hoko, H., Ishikawa, H., Fukui, Y (1990), Int. J. Infrared Milllimeter Waves in press.Google Scholar
Fukui, Y. (1989), Low Mass Star Formation and Pre-Main Sequence Objects , Reipurth, B. (ed.) (ESO: Garching) p. 141.Google Scholar