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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© 1994 Springer Science+Business Media Dordrecht
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Rawlings, J.M.C., Evans, N.J., Zhou, S. (1994). Gas-Grain Interaction in the Low Mass Star-Forming Region B335. In: Dyson, J.E., Carling, E.B. (eds) Kinematics and Dynamics of Diffuse Astrophysical Media. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0926-0_27
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DOI: https://doi.org/10.1007/978-94-011-0926-0_27
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4399-1
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