Formation of planetary populations − II. Effects of initial disc size and radial dust drift
ABSTRACT Recent ALMA observations indicate that while a range of disc sizes exist, typical disc radii are small, and that radial dust drift affects the distribution of solids in discs. Here, we explore the consequences of these features in planet population synthesis models. A key feature of our mod...
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Published in | Monthly notices of the Royal Astronomical Society Vol. 493; no. 1; pp. 1013 - 1033 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Oxford University Press
01.03.2020
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Subjects | |
Online Access | Get full text |
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