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Observations of high co rotational lines in post-AGBs and PN

  • Session G: AGB Stars, Proto-Planetary Nebulae & Planetary Nebulae
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Abstract

We present a preliminary interpretation of high CO rotational line data obtained from KAO. The possibility of either a PDR or a shock model is considered in order to explain the observations.

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Authors and Affiliations

  1. NASA Ames Research Center, MS 245-3, 94035, Moffett Field, CA, USA

    K. Justtanont & A. G. G. M. Tielens

  2. L-413, Lawrence Livermore National Laboratory, IGPP, PO Box 808, 94551, Livermore, CA, USA

    C. J. Skinner

  3. NASA Ames Research Center, MS 245-6, 94035, Moffett Field, CA, USA

    M. R. Haas

Authors
  1. K. Justtanont
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  2. A. G. G. M. Tielens
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  3. C. J. Skinner
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  4. M. R. Haas
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Justtanont, K., Tielens, A.G.G.M., Skinner, C.J. et al. Observations of high co rotational lines in post-AGBs and PN. Astrophys Space Sci 224, 305–308 (1995). https://doi.org/10.1007/BF00667862

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  • DOI: https://doi.org/10.1007/BF00667862

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