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. Author manuscript; available in PMC: 2020 Jun 19.
Published in final edited form as: Astron Astrophys. 2020 May 12;637:A39. doi: 10.1051/0004-6361/201937180

Fig. 10.

Fig. 10

Plots that show the predicted abundances (solid lines) of the CS (top row), H2S (middle row), and SO (bottom row) by models with different chemical desorption schemes, together with the observed abundances in Barnard 1b, at times 0.1 − 1 − 10 Myrs. The vertical dashed line represents Av = 8 mag, and the shaded area encloses the range of extinctions 6 − 19 mag.