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Temperature gradients across the Rho Oph B1/B2 molecular core: The effects of heating by low luminosity stars on cloud cores

  • Molecular Cloud Properties
  • Conference paper
  • First Online:
Molecular Clouds in the Milky Way and External Galaxies

Part of the book series: Lecture Notes in Physics ((LNP,volume 315))

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References

  • Herbst, E. 1982, Astr. Ap., 111, 76.

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  • Wilson, R. W., Langer, W. D., and Goldsmith, P. F. 1981, Ap. J. (Letters), 243, L47.

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  • Wootten, A., Loren, R. B., and Snell, R. L. 1982, Ap. J., 255, 160.

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Authors
  1. H. Butner
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  2. R. Loren
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  3. Alwyn Wootten
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  4. N. Kaifu
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  5. H. Suzuki
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  6. T. Yamashita
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  7. S. Hayashi
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Editor information

Robert L. Dickman Ronald L. Snell Judith S. Young

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© 1988 Springer-Verlag

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Butner, H. et al. (1988). Temperature gradients across the Rho Oph B1/B2 molecular core: The effects of heating by low luminosity stars on cloud cores. In: Dickman, R.L., Snell, R.L., Young, J.S. (eds) Molecular Clouds in the Milky Way and External Galaxies. Lecture Notes in Physics, vol 315. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-50438-9_227

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  • DOI: https://doi.org/10.1007/3-540-50438-9_227

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-50438-2

  • Online ISBN: 978-3-540-46003-9

  • eBook Packages: Springer Book Archive

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