Chapter 44. CNO Abundances in the Quintuplet Cluster M Supergiant 5–7

  1. Dr. A. Cotera4,
  2. Dr. S. Markoff5,
  3. T. R. Geballe7 and
  4. Prof. Dr. H. Falcke6
  1. S. V. Ramirez1,
  2. K. Sellgren2,
  3. R. Blum3 and
  4. D. M. Terndrup2

Published Online: 30 DEC 2007

DOI: 10.1002/9783527617982.ch44

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

Ramirez, S. V., Sellgren, K., Blum, R. and Terndrup, D. M. (2007) CNO Abundances in the Quintuplet Cluster M Supergiant 5–7, 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.ch44

Editor Information

  1. 4

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

  2. 5

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

  3. 6

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

  4. 7

    Gemini Observatory, tgeballe@gemini.edu

Author Information

  1. 1

    Infrared Processing and Analysis Center, California Institute of Technology, Mail Code 100–22, 770 South Wilson Avenue, Pasadena, CA 91125, USA

  2. 2

    Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 USA

  3. 3

    NOAO/CTIO, Casilla 603, La Serena, Chile

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:

  • stars;
  • abundances;
  • Galactic center;
  • formation;
  • blended

Summary

This chapter contains sections titled:

  • Introduction

  • Observations and Analysis

  • Results and discussion