Molecular Diagnostics of Diffusive Boundary Layers

Details Molecular Diagnostics of Diffusive Boundary Layers Molecular Diagnostics of Diffusive Boundary Layers

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...487..672r&link_type=abstract

Astrophysical Journal v.487, p.672

Astronomy and Astrophysics

Astronomy

17

Ism: Bubbles, Stars: Pre-Main-Sequence, Ism: Jets And Outflows, Ism: Molecules

Scientific paper

We have examined the chemistry in thin (<~0.01 pc) boundary layers between dark star-forming cores and warm, shocked T Tauri winds on the assumption that turbulence-driven diffusion occurs within them. The results indicate that emissions from C+, CH, OH, H2O and the J = 6 --> 5 transition of CO, among others, may serve as diagnostics of the boundary layers.

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