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Velocity Gradient in the Presence of Self-gravity: Identifying Gravity-induced Inflow and Determining Collapsing Stage

  • Authors: Yue Hu, A. Lazarian, and Ka Ho Yuen

2020 The Astrophysical Journal 897 123.

  • Provider: AAS Journals

Caption: Figure 13.

Panel (a): the first and second rows are two subregions extracted from simulation A1 at tr ≃ 0.8 Myr, denoted as A1-1 (length scale ≃1.7 pc) and A1-2 (length scale ≃2.8 pc), respectively. First column: gravitationally collapsing regions (blue regions) identified from the N-PDFs. Second column: orientation of velocity gradients in the range of [0, π] (i.e., red: ≃π, blue: ≃0, and green: ≃π/2). Third column: projected velocity convergence of each corresponding region. Discontinuity comes from numerical effect. Panel (b): gravitationally collapsing regions (red regions) identified from the double-peak feature of velocity gradients' morphology. Second block size is implemented in the double-peak algorithm to plot the histogram of velocity gradients’ orientation in a subregion. We test three block sizes: 30, 40, and 50 pixels.

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