Skip to main content
. 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. 3.

Fig. 3

Observed H2S gas-phase abundance plotted against ngasT(cm3K1/2) in log scale, showing the sticking behavior described by Eq. (1). Crosses mark upper bound values, which were not taken into account in this analysis.