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Fig. 3.

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Grid of log density slices of stars of ∼20 tdyn, ⋆ after undergoing μTDEs, with the BH at the center of each panel. Each row is for a different mBH (top and bottom half for 10 M and 40 M, respectively), m, or Hc, whereas the columns represent increasing b (from left to right). The dashed and solid circles around the BH, most visible in the rightmost panels, denote the tidal radius, rt, and the periapsis distance, rp, respectively. We note that the spatial range of each panel is not the same.

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