Chapter 60. Closure Amplitude Analysis of 15, 22 and 43 GHz VLBA Observations of Sagittarius A*: Size is Consistent with the Scattering Law

  1. Dr. A. Cotera2,
  2. Dr. S. Markoff3,
  3. T. R. Geballe5 and
  4. Prof. Dr. H. Falcke4
  1. G. C. Bower

Published Online: 30 DEC 2007

DOI: 10.1002/9783527617982.ch60

Proceedings of the Galactic Center Workshop 2002: The Central 300 parsecs of the Milky Way

Proceedings of the Galactic Center Workshop 2002: The Central 300 parsecs of the Milky Way

How to Cite

Bower, G. C. (2003) Closure Amplitude Analysis of 15, 22 and 43 GHz VLBA Observations of Sagittarius A*: Size is Consistent with the Scattering Law, in Proceedings of the Galactic Center Workshop 2002: The Central 300 parsecs of the Milky Way (eds A. Cotera, S. Markoff, T. R. Geballe and H. Falcke), Wiley-VCH Verlag GmbH, Weinheim, Germany. doi: 10.1002/9783527617982.ch60

Editor Information

  1. 2

    SETI Institute, Arizona State University, cotera@asu.edu

  2. 3

    Max Planck Institute, Center for Space Research, smarkoff @ mpifr-bonn.mpg.de

  3. 4

    Max Planck Institute, Center for Space Research, falcke@astron.nl

  4. 5

    Gemini Observatory, tgeballe@gemini.edu

Author Information

  1. Radio Astronomy Lab, UC Berkeley, Berkeley CA 94720

Publication History

  1. Published Online: 30 DEC 2007
  2. Published Print: 17 DEC 2003

ISBN Information

Print ISBN: 9783527404667

Online ISBN: 9783527617982

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Keywords:

  • amplitude;
  • technique;
  • VLBA;
  • unbiasing;
  • synthesized

Summary

This chapter contains sections titled:

  • The Size of Sagittarius A*

  • VLBA Observations and Analysis

  • Closure Amplitude Results