Fig. 8
Inferred disk mass distribution for the NGC 2024 disk population (dark red) and the hypothesized western and eastern subpopulations, in tan and green respectively. The dividing line between these populations runs from 5:41:44.189 −1°55′39.94″ and 5:41:38.665 -1°53′00.27″, tangentially to the southern part of the dense molecular ridge.
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