Image Details
Caption: Figure 9.
Early rise-time τ rise (top) and late-time slope n ∞ (bottom) for ZAMS (left) and TAMS (right) stars for different M ⋆, a, and β. The “+” and “-” symbols indicate the results from the disruptions of stars on prograde and retrograde orbits, respectively. The results for the GR and NR simulations are indicated with “•” and “▪” symbols, respectively. For partial disruption the analytically predicted slope is n ∞ ≈ − 9/4 and for total disruption it is n ∞ ≈ − 5/3, which are represented with a dashed and a dashed–dotted line, respectively.
© 2023. The Author(s). Published by the American Astronomical Society.