A simple model for the evolution of the dust population in protoplanetary disks

DOI10.1051/0004-6361/201118136zbMath1260.85032arXiv1201.5781OpenAlexW2041172302WikidataQ69024887 ScholiaQ69024887MaRDI QIDQ4905994

Tilman Birnstiel, B. Ercolano, H. Klahr

Publication date: 21 February 2013

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1201.5781

zbMATH Keywords

accretion diskscircumstellar matterprotoplanetary disksplanets and satellites: formationstars: pre-main sequence

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Stability and instability of geophysical and astrophysical flows (76E20) Statistical astronomy (85A35)

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