Fig. 16.
Resulting logarithmic abundance corrections Δ log AO by the mini–curves-of-growth of the H2O blends in 2MASS 1835+32 plotted against the observed values of log (W/λ)obs. A dashed line shows the mean correction. (a) Based on the dusty model Bc2280c526 and Vrotsin i = 40.8 km s−1. (b) Based on the dust-free model Cc2280c526 and Vrotsin i = 40.8 km s−1. (c) Based on the dusty model Bc2280c526 and Vrotsin i = 37.6 km s−1. (d) Based on the dusty model Bc2280c526 and Vrotsin i = 44.0 km s−1. (e) Based on the dusty model Bc2180c528 and Vrotsin i = 40.8 km s−1. (f) Based on the dusty model Bc2380c525 and Vrotsin i = 40.8 km s−1. (Color online)

Resulting logarithmic abundance corrections Δ log AO by the mini–curves-of-growth of the H2O blends in 2MASS 1835+32 plotted against the observed values of log (W/λ)obs. A dashed line shows the mean correction. (a) Based on the dusty model Bc2280c526 and Vrotsin i = 40.8 km s−1. (b) Based on the dust-free model Cc2280c526 and Vrotsin i = 40.8 km s−1. (c) Based on the dusty model Bc2280c526 and Vrotsin i = 37.6 km s−1. (d) Based on the dusty model Bc2280c526 and Vrotsin i = 44.0 km s−1. (e) Based on the dusty model Bc2180c528 and Vrotsin i = 40.8 km s−1. (f) Based on the dusty model Bc2380c525 and Vrotsin i = 40.8 km s−1. (Color online)

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