Hostname: page-component-76fb5796d-skm99 Total loading time: 0 Render date: 2024-04-26T20:16:06.023Z Has data issue: false hasContentIssue false
  • English
  • Français

VLBI Observations of the Gravitational Lens System 2016+112

Published online by Cambridge University Press:  03 August 2017

M. B. Heflin ,
M. V. Gorenstein ,
E. E. Falco ,
I. I. Shapiro ,
B. F. Burke ,
J. N. Hewitt ,
A. E. E. Rogers  and
C. R. Lawrence
M. B. Heflin
Affiliation:
MIT
M. V. Gorenstein
Affiliation:
CfA
E. E. Falco
Affiliation:
CfA
I. I. Shapiro
Affiliation:
CfA
B. F. Burke
Affiliation:
MIT
J. N. Hewitt
Affiliation:
Haystack
A. E. E. Rogers
Affiliation:
Haystack
C. R. Lawrence
Affiliation:
CIT

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.

On June 1, 1984 we conducted a seven station 18-cm VLBI observation of the 2016+112 gravitational lens system. Preliminary brightness distributions for A and B have been obtained via model fitting. Weak correlated flux density was detected in the C component region.

Type
Extragalactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 209 - 210
Copyright
Copyright © Reidel 1988 

References

1. Lawrence, C. R., et al. 1984, Science 223, 46.CrossRefGoogle Scholar
2. Schneider, D. P., et al. 1985, Ap. J. 294, 66.Google Scholar
3. Gorenstein, M. V., et al. 1984, Ap. J. 287, 538.Google Scholar
4. Gorenstein, M. V., et al. 1983, Science 219, 54.Google Scholar