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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2 Pith papers cite this work. Polarity classification is still indexing.
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Planet-hosting wide binaries display diverse differential abundance trends with condensation temperature that are not universal across systems.
citing papers explorer
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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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Chemical signatures of planetary systems in their host stars. Near-infrared spectroscopy of four planet-hosting wide binaries
Planet-hosting wide binaries display diverse differential abundance trends with condensation temperature that are not universal across systems.