Hostname: page-component-cb9f654ff-65tv2 Total loading time: 0 Render date: 2025-08-08T04:30:37.099Z Has data issue: false hasContentIssue false
  • English
  • Français

The Molonglo 843 MHz survey of the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

A. J. Turtle  and
S. W. Amy
A. J. Turtle
Affiliation:
School of Physics, University of Sydney NSW 2006, Australia
S. W. Amy
Affiliation:
School of Physics, University of Sydney NSW 2006, Australia

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.

A radio survey of the Magellanic Clouds (MCs) at 843 MHz has been completed and is being prepared for publication. The survey was made with the Molonglo Observatory Synthesis Telescope (MOST) operated by the Astrophysics Department, University of Sydney. This survey of the Clouds has a high angular resolution (45 arcsec) and a sensitivity of a few mJy/beam even for objects of large angular extent

Information

Type
Large-Scale Structure and Kinematics
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 114 - 115
Copyright
Copyright © Kluwer 1991 

References

Davies, R.D., Elliott, K.H., Meaburn, J. (1976), Mem. R. astr. Soc. 81, 89.Google Scholar
Mills, B.Y. (1981), Proc. Astron. Soc. Aust. 4, 156.CrossRefGoogle Scholar
Mills, B.Y., Turtle, A.J., Little, A.G., Durdin, J.M. (1984), Aust. J. Phys. 37, 321.CrossRefGoogle Scholar
Ye, T. (1988), PhD Thesis, University of Sydney.Google Scholar