The accumulation and trapping of grains at planet gaps: Effects of grain growth and fragmentation
Open Access
- 1 October 2015
- journal article
- research article
- Published by Elsevier in Planetary and Space Science
- Vol. 116, 48-56
Abstract
No abstract availableKeywords
All Related Versions
This publication has 53 references indexed in Scilit:
- Characterization of global flow and local fluctuations in 3D SPH simulations of protoplanetary discsMonthly Notices of the Royal Astronomical Society, 2013
- Flows of gas through a protoplanetary gapNature, 2013
- On the accumulation of planetesimals near disc gaps created by protoplanetsMonthly Notices of the Royal Astronomical Society, 2012
- FORMATION OF GIANT PLANETS BY DISK INSTABILITY ON WIDE ORBITS AROUND PROTOSTARS WITH VARIED MASSESThe Astrophysical Journal, 2011
- Gas- and dust evolution in protoplanetary disksAstronomy & Astrophysics, 2010
- The Growth Mechanisms of Macroscopic Bodies in Protoplanetary DisksAnnual Review of Astronomy and Astrophysics, 2008
- Coagulation, fragmentation and radial motion of solid particles in protoplanetary disksAstronomy & Astrophysics, 2007
- Dust distribution in protoplanetary disksAstronomy & Astrophysics, 2005
- Models of giant planet formation with migration and disc evolutionAstronomy & Astrophysics, 2005
- Tidally Induced Gap Formation in Protostellar Disks: Gap Clearing and Suppression of Protoplanetary GrowthThe Astrophysical Journal, 1999