Image Details
Caption: Figure C2.
Similar to Figure 2, but for the models neglecting the cloud phase (i.e., α = 0). The top, middle, and bottom panels correspond to the initial H2 OPR of 10−3, 10−2, and 10−1, respectively. From left to right, the metallicity decreases from Z = 1 to 0.2. The core density is 105 cm−3 in all the models.
© 2026. The Author(s). Published by the American Astronomical Society.