Chapter 65. The wavelength dependence of Sgr A* size and the unified model of compact radio sources

  1. Dr. A. Cotera2,
  2. Dr. S. Markoff3,
  3. T. R. Geballe5 and
  4. Prof. Dr. H. Falcke4
  1. Fedor Prigara

Published Online: 30 DEC 2007

DOI: 10.1002/9783527617982.ch65

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

Prigara, F. (2003) The wavelength dependence of Sgr A* size and the unified model of compact radio sources, 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.ch65

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. Institute of Microelectronics and Informatics, Russian Academy of Sciences, 21 Universitetskaya, Yaroslavl 150007, Russia

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:

  • Galaxy: center;
  • radio continuum;
  • galactic;
  • amplification;
  • nuclei

Summary

This chapter contains sections titled:

  • Introduction

  • The gaseous disk model

  • Extended radio sources

  • The wavelength dependence of radio source size

  • Maser amplification of thermal radio emission

  • Conclusions