Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-06T06:58:34.065Z Has data issue: false hasContentIssue false

A radio source model based on measurements of polarization and brightness distribution

Published online by Cambridge University Press:  16 November 2021

A. T. Moffet*
Affiliation:
Owens Valley Radio Observatory, California Institute of Technology, Pasadena, Calif., U.S.A.

Abstract

Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Part 4 Joint Discussions
Copyright
Copyright © Academic Press 1966 

References

1. Seielstad, G. A., Morris, D., Radhakrishnan, V. Astrophys. J., 140, 53, 1964.Google Scholar
2. Morris, D., Berge, G. L. Astr. J., 69, 641, 1964.Google Scholar
3. Moffet, A. T. Science, 146, 764, 1964.Google Scholar
1. Greyber, H. D. Bull. Am. phys. Soc, 6, 285, 1961.Google Scholar
2. Greyber, H. D. Trans. IAU, 11, 332, 1961.Google Scholar
3. Greyber, H. D. U.S. AFOSR Res. Rep. no. 2158, June 1962.Google Scholar
4. Elvius, A. Bull. Lowell Obs. no. 119, 1962.Google Scholar
5. Lynds, C., Sandage, A. Astrophys. J., 137, 1005, 1963.Google Scholar
6. Morris, D., Berge, G. Astrophys. J., 139, 1388, 1964.Google Scholar
7. Greyber, H. D. 116th Meeting of the American Astronomical Society, Flagstaff, Arizona, Abstract 51a, June 1964.Google Scholar