Hostname: page-component-8448b6f56d-c47g7 Total loading time: 0 Render date: 2024-04-24T23:12:53.058Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

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