Radiation hydrodynamic simulations of wind-reprocessed TDEs reveal a ~3-week offset between optical/UV and bolometric light curve peaks due to the buildup time of the reprocessing layer.
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Strange quark matter strangelets with low baryon number can form stable self-gravitating sub-stellar objects, predicting a new class of ultra-compact candidates with a density gap from ordinary planets and brown dwarfs.
citing papers explorer
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The Light Curve of Wind-Reprocessed Tidal Disruption Events
Radiation hydrodynamic simulations of wind-reprocessed TDEs reveal a ~3-week offset between optical/UV and bolometric light curve peaks due to the buildup time of the reprocessing layer.
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Sub-stellar Strange Quark Matter Objects: Predicting a New Class of Highly-Compact Candidates
Strange quark matter strangelets with low baryon number can form stable self-gravitating sub-stellar objects, predicting a new class of ultra-compact candidates with a density gap from ordinary planets and brown dwarfs.