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Jet–Environment Interaction after Delayed Collapse in Binary Neutron Star Mergers
Jay V. Kalinani et al 2026 The Astrophysical Journal Letters 1000 .
Caption: Figure 5.
Rest-mass density profiles along the z-axis (south side) for cases C and D, at 1 ms or 26 ms after BH formation.
© 2026. The Author(s). Published by the American Astronomical Society.
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