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Towards an Understanding of the Galactic Distribution of Electron-Density Fluctuations

Published online by Cambridge University Press:  12 April 2016

J. F. Salgado ,
C. J. Salter ,
T. Ghosh ,
W. Junor  and
P. K. Manoharan
J. F. Salgado
Affiliation:
University of Michigan, Dept. of Astronomy, Ann Arbor, MI 48109-1090, USA
C. J. Salter
Affiliation:
NAIC, Arecibo Observatory, P.O. Box 995, Arecibo, PR 00613, USA
T. Ghosh
Affiliation:
NAIC, Arecibo Observatory, P.O. Box 995, Arecibo, PR 00613, USA
W. Junor
Affiliation:
Dept. of Phys. & Astr., Univ. of New Mexico, Albuquerque, NM 87131, USA
P. K. Manoharan
Affiliation:
Radio Astronomy Centre, TIFR, P.O. Box 8, Ooty 643001, India

Abstract

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VLBA observations of 32 compact sources within 30° ≤ ᶩ ≤ 75°, | b | < 3° are being used to test whether the galactic electron-density fluctuations contain a spiral component.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 287 - 288
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Fey, A.L., Spangler, S.R., & Cordes, J.M. 1991. ApJ, 372, 132–160.CrossRefGoogle Scholar
Ghosh, T., & Rao, A.P. 1992. A&A, 264, 203–216.Google Scholar
Taylor, J.H., & Cordes, J.M. 1993. ApJ, 411, 674–684.CrossRefGoogle Scholar