Fig. 9
Midplane water snowline as a function of stellar luminosity, accretion rate, and disk radius. The envelope mass is fixed at 1 M⊙ with a disk mass of 0.1 M⊙ and Rcen = 200 AU. The different panels show the water snowline as a function of stellar luminosity: 1 L⊙ (left), 5 L⊙ (center), and 15 L⊙ (right). The different colors indicate the disk radius: 200 AU (blue), 100 AU (green), and 50 AU (red).
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