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Gas-grain interaction in the low mass star-forming region B335

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Abstract

We have modelled chemical abundances and line profiles in the Bok globule B335. The chemical characteristics of this star-forming core are largely determined by gas-grain interaction in the inflowing material. By comparing high resolution observational data with our model it should be possible to determine the evolutionary status of B335 and to establish the role that surface chemistry plays in protostellar clouds.

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Authors and Affiliations

  1. Department of Mathematics, UMIST, PO Box 88, M60 1QD, Manchester, UK

    J. M. C. Rawlings

  2. Department of Astronomy, The University of Texas at Austin, Austin, Texas, USA

    N. J. Evans II & S. Zhou

Authors
  1. J. M. C. Rawlings
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  2. N. J. Evans II
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  3. S. Zhou
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Rawlings, J.M.C., Evans, N.J. & Zhou, S. Gas-grain interaction in the low mass star-forming region B335. Astrophys Space Sci 216, 155–157 (1994). https://doi.org/10.1007/BF00982487

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  • DOI: https://doi.org/10.1007/BF00982487

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