Chapter 70. A model for polarised radio emission from Sgr A*

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

Published Online: 30 DEC 2007

DOI: 10.1002/9783527617982.ch70

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

Beckert, T. (2003) A model for polarised radio emission from Sgr A*, 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.ch70

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. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany

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:

  • Plasmas;
  • radiative transfer;
  • polarization;
  • Galaxy: center;
  • frequency

Summary

This chapter contains sections titled:

  • Introduction

  • Representation of the radiation field

  • Outflow Model

  • Radiative Transfer Effects

  • Two drivers for source intrinsic conversion

  • Results - Application to Sgr A*

  • Conclusions