Chapter 88. Hot Molecular Gas in the Central 10 Parsecs of the Galaxy

  1. Dr. A. Cotera2,
  2. Dr. S. Markoff3,
  3. T. R. Geballe5 and
  4. Prof. Dr. H. Falcke4
  1. R. M. Herrnstein and
  2. P. T. P. Ho

Published Online: 30 DEC 2007

DOI: 10.1002/9783527617982.ch88

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

Herrnstein, R. M. and Ho, P. T. P. (2003) Hot Molecular Gas in the Central 10 Parsecs of the Galaxy, 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.ch88

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. MS-10, 60 Garden St., Cambridge, MA 02138

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:

  • Galactic Center;
  • ISM;
  • radio lines;
  • supermassive;
  • transitions

Summary

This chapter contains sections titled:

  • Introduction

  • Observations and Data Reduction

  • The Effect of Sgr A East on the Molecular Environment

  • Hot Molecular Gas near Sgr A*