AGN dust tori can form tens of millions of planetesimals from Earth to super-Jupiter masses via streaming instability, with continued growth to stellar masses through pebble and gas accretion.
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MOFAT applied to SN2024ggi shows CO triggering inner SiO formation with a receding edge, order-of-magnitude mass drop, clumping signatures, and no dust formation.
Numerical models of fast radiation-mediated shocks and planar shock breakout show that including bound-free and bound-bound opacities from solar-composition heavy elements maintains local thermal equilibrium to higher velocities and reduces breakout emission temperatures by factors of two to ten.
Free neutrons survive r-process freeze-out in fast ejecta of neutron star mergers and their beta-decay heating produces a visible early kilonova precursor for mass fractions above ~0.05.
citing papers explorer
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Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets
AGN dust tori can form tens of millions of planetesimals from Earth to super-Jupiter masses via streaming instability, with continued growth to stellar masses through pebble and gas accretion.
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Probing the 3D Structures of Supernovae through IR Signatures of CO and SiO
MOFAT applied to SN2024ggi shows CO triggering inner SiO formation with a receding edge, order-of-magnitude mass drop, clumping signatures, and no dust formation.
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Radiation Mediated Shock and Planar Shock Breakout in the Presence of Atomic Transition Lines
Numerical models of fast radiation-mediated shocks and planar shock breakout show that including bound-free and bound-bound opacities from solar-composition heavy elements maintains local thermal equilibrium to higher velocities and reduces breakout emission temperatures by factors of two to ten.
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Nucleosynthesis in the fast ejecta of a neutron star merger
Free neutrons survive r-process freeze-out in fast ejecta of neutron star mergers and their beta-decay heating produces a visible early kilonova precursor for mass fractions above ~0.05.