Chapter 86. Physical Conditions in the Central Parsec Modeled from Mid-Infrared Imaging Photometry

  1. Dr. A. Cotera3,
  2. Dr. S. Markoff4,
  3. T. R. Geballe6 and
  4. Prof. Dr. H. Falcke5
  1. Dan Gezari1,
  2. Eli Dwek1 and
  3. Frank Varosi2

Published Online: 30 DEC 2007

DOI: 10.1002/9783527617982.ch86

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

Gezari, D., Dwek, E. and Varosi, F. (2003) Physical Conditions in the Central Parsec Modeled from Mid-Infrared Imaging Photometry, 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.ch86

Editor Information

  1. 3

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

  2. 4

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

  3. 5

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

  4. 6

    Gemini Observatory, tgeballe@gemini.edu

Author Information

  1. 1

    NASA/Goddard Space Flight Center, Infrared Astrophysics Branch, Code 685, Greenbelt, MD 20771 USA

  2. 2

    University of Florida, Department of Astronomy, Gainsville, FL 32611 USA

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:

  • infrared;
  • imaging;
  • galactic center;
  • luminosity;
  • radiation

Summary

This chapter contains sections titled:

  • Introduction

  • Dust Emission-Extinction Model

  • Discussion

  • Conclusions