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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 21.

Top: visualization of 3D velocity convergence using simulation A1 at tr ≃ 0.8 Myr. Positive convergence outlines the convergent inflow. Inner blue box approximately outlines the boundary of the 3D collapsing region identified from IGT. Projected 2D plot on the right side shows the corresponding intensity gradients amplitude log ﹩(| {\rm{\nabla }}I| )﹩. We mask the low-amplitude pixel, i.e., its corresponding amplitude is less than the global mean value. Middle: visualization of 3D intensity structures. Inner blue box approximately outlines the boundary of the 3D collapsing region identified from IGT (red region in the 2D projection). We highlight high-intensity structures, i.e., their corresponding intensity is five times larger than the global mean value. Bottom: visualization of 3D gravitational energy. Inner blue box approximately outlines the boundary of the 3D collapsing region identified from VGT (red region in the 2D projection). We keep only the pixels with high gravitational energy, i.e., those with corresponding gravitational energy five times larger than the global mean value.

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