Chapter 41. Simulated X-ray emission from the Arches cluster

  1. Dr. A. Cotera5,
  2. Dr. S. Markoff6,
  3. T. R. Geballe8 and
  4. Prof. Dr. H. Falcke7
  1. Pablo F. Velázquez1,
  2. Alejandro C. Raga1,
  3. Jorge Cantó2,
  4. Elena Masciadri3 and
  5. Luis F. Rodríguez4

Published Online: 30 DEC 2007

DOI: 10.1002/9783527617982.ch41

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

Velázquez, P. F., Raga, A. C., Cantó, J., Masciadri, E. and Rodríguez, L. F. (2003) Simulated X-ray emission from the Arches cluster, 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.ch41

Editor Information

  1. 5

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

  2. 6

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

  3. 7

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

  4. 8

    Gemini Observatory, tgeballe@gemini.edu

Author Information

  1. 1

    Instituto de Ciencias Nucleares, UNAM, Apdo. Postal 70-543, CP 04510, México D.F., México.

  2. 2

    Instituto de Astronomía, UNAM, Apdo. Postal 70-264, CP 04510, México D.F., México.

  3. 3

    Max-Plank-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany

  4. 4

    Instituto de Astronomía, UNAM, campus Morelia, Apdo. Postal 3-72, Morelia, Michoacán, CP 58089, México

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;
  • hydrodynamics;
  • methods: numerical;
  • open clusters and associations: individual (Arches;
  • G0.121+0.017);
  • shock waves;
  • stars: winds;
  • outflows

Summary

This chapter contains sections titled:

  • Introduction

  • A model for the Arches cluster

  • Numerical simulation

  • Results

  • Conclusions