Kinematics of young stellar objects in NGC 2024 based on infrared proper motions

Open Access

Fig. 12

Location of the center of NGC 2024 (white square) and the PV diagram path (red line) for Figs. 13 and 14. The panels show a cutout of the VHS K_s-band observation, and the maximum gas temperature for the (1 - 0) molecular transitions of N₂H⁺, HNC, and HCN.

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