Preprint
Dust in Protoplanetary Disks: A Clue as to the Critical Mass of Planetary Cores
Abstract
Dust in protoplanetary disks is recognized as the building blocks of planets.
In the core accretion scenario, the abundance of dust in disks (or metallicity)
Authors
Hasegawa Y; Pudritz RE
Publication date
January 30, 2014
DOI
10.48550/arxiv.1401.7845
Preprint server
arXiv