Sulfur gas-phase abundance in dense cores | Astronomy & Astrophysics (A&A)

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Fig. 6

Steady-state abundance of NS and N₂H⁺ from our grids of models (top: n₄ = 1; bottom: n₄ = 10) are compared to the observational estimates listed in Table 2. The value of n₄, ζ₁₇, and the ratioζ₁₇∕n₄ are indicated in each panel. Five values of S_gas (see Table 3) are associated with each C/O ratio.

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