A new Bessel kernel for 2D disc gravity fixes convergence in GI simulations and reveals that softening prescriptions overestimate formed planet masses by a factor of 2-3.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Protoplanetary disc lifetime distributions are mass-dependent, peaking at 3.72 Myr for high-mass stars and 7.20 Myr for low-mass stars when modeled with Weibull fits assuming an initial disc fraction of 0.8.
PS16dtm is the tidal disruption of a 0.3 solar-mass star on a circular counter-rotating orbit inside the accretion disk of an NLS1 galaxy, hidden by a gaseous envelope from the observer's view.
citing papers explorer
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Self-gravity in thin protoplanetary discs: 2. Numerical convergence solved and revealing the overestimation in mass of formed planets with softening
A new Bessel kernel for 2D disc gravity fixes convergence in GI simulations and reveals that softening prescriptions overestimate formed planet masses by a factor of 2-3.
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Disc lifetime distribution as a function of the mass of host star
Protoplanetary disc lifetime distributions are mass-dependent, peaking at 3.72 Myr for high-mass stars and 7.20 Myr for low-mass stars when modeled with Weibull fits assuming an initial disc fraction of 0.8.
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Tidal disruption of a low-mass star in an active galactic nucleus as the origin of the PS16dtm outburst
PS16dtm is the tidal disruption of a 0.3 solar-mass star on a circular counter-rotating orbit inside the accretion disk of an NLS1 galaxy, hidden by a gaseous envelope from the observer's view.