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Synthetic specira for the n-type carbon star TX Psc

  • Heating of Stellar Chromospheres and Coronae
  • Conference paper
  • First Online:
Cool Stars, Stellar Systems, and the Sun

Part of the book series: Lecture Notes in Physics ((LNP,volume 291))

  • 159 Accesses

Abstract

Initial modeling of TX Psc's chromosphere is presented. Simple LTE flux calculations can be made to reproduce the IUE spectrum. Non-LTE effects of hydrogen decrease the electron density in the outer layers as compared to LTE.

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References

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Author information

Authors and Affiliations

  1. Dept. of Astronomy, Indiana University, 47401, Bloomington, IN

    Donald G. Luttermoser & Hollis R. Johnson

  2. Center for Astrophysics, 02138, Cambridge, MA

    Eugene H. Avrett & Rudolf Loeser

Authors
  1. Donald G. Luttermoser
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  2. Hollis R. Johnson
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  3. Eugene H. Avrett
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  4. Rudolf Loeser
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Editor information

Jeffrey L. Linsky Robert E. Stencel

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© 1987 Springer-Verlag

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Luttermoser, D.G., Johnson, H.R., Avrett, E.H., Loeser, R. (1987). Synthetic specira for the n-type carbon star TX Psc. In: Linsky, J.L., Stencel, R.E. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 291. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-18653-0_127

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  • DOI: https://doi.org/10.1007/3-540-18653-0_127

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-18653-3

  • Online ISBN: 978-3-540-48041-9

  • eBook Packages: Springer Book Archive

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