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Three Micron Spectra of Carbon Stars in the Large Magellanic Cloud

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Mass-Losing Pulsating Stars and their Circumstellar Matter

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 283))

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Abstract

Infrared spectra of six carbon-rich stars were obtained with the Very Large Telescope (VLT). We found a metallicity dependence in the equivalent width of the molecular bands, and we discuss the causes of this

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Author information

Authors and Affiliations

  1. Department of Physics, UMIST, P.O. Box 88, Manchester, M60 1QD, UK

    M. Matsuura, A.A Zijlstra & A.J Markwick

  2. School of Chemistry and Physics, Keele University, Staffordshire, ST5 5BG, UK

    J.Th van Loon

  3. The Institute of Space and Astronautical Science, Kanagawa, 229-8510, Japan

    I. Yamamura

  4. European Southern Observatory, Alonso de Cordova 3107, Casilla, 19001, Santiago 19, Chile & UMIST, UK

    Paul M. Woods

Authors
  1. M. Matsuura
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  2. A.A Zijlstra
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  3. A.J Markwick
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  4. J.Th van Loon
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  5. I. Yamamura
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  6. Paul M. Woods
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Editor information

Editors and Affiliations

  1. Kiso Observatory, University of Tokyo, Agematsu, Japan

    Y. Nakada

  2. National Astronomical Observatory, Mitaka, Japan

    M. Honma

  3. Astronomical Institute, Tohoku University, Sendai, Japan

    M. Seki

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© 2003 Springer Science+Business Media Dordrecht

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Matsuura, M., Zijlstra, A., Markwick, A., van Loon, J., Yamamura, I., Woods, P.M. (2003). Three Micron Spectra of Carbon Stars in the Large Magellanic Cloud. In: Nakada, Y., Honma, M., Seki, M. (eds) Mass-Losing Pulsating Stars and their Circumstellar Matter. Astrophysics and Space Science Library, vol 283. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0139-7_63

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  • DOI: https://doi.org/10.1007/978-94-010-0139-7_63

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-3968-0

  • Online ISBN: 978-94-010-0139-7

  • eBook Packages: Springer Book Archive

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