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Fig. 4

image

Radial profiles of water ice fractional abundances /nH in NGC1333-IRAS 2A (left panel) and NGC 1333-IRAS 4A (right panel) envelope models. The line color gradually changes from green to cyan, blue, and indigo as the value of LX increases. The profiles for LX = 0−1029 erg s−1 almost overlap. In Figs. 7, C.1, and C.2, we adopt the same line types and color patterns of the radial fractional abundance profiles of icy-phase molecules for different values of LX.

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