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

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

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216..155r&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 155-157

Astronomy and Astrophysics

Astrophysics

4

Abundance, Interplanetary Dust, Interstellar Chemistry, Molecular Clouds, Protostars, Star Formation, Stellar Composition, Stellar Models, Line Spectra, Stellar Envelopes, Stellar Evolution, Stellar Spectra

Scientific paper

We have modeled 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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