The Citing articles tool gives a list of articles citing the current article. The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Daniel Mentiplay, Daniel J Price and Christophe Pinte Monthly Notices of the Royal Astronomical Society: Letters 484(1) L130 (2019) https://doi.org/10.1093/mnrasl/sly209
The formation of Jupiter’s diluted core by a giant impact
Shang-Fei Liu, Yasunori Hori, Simon Müller, Xiaochen Zheng, Ravit Helled, Doug Lin and Andrea Isella Nature 572(7769) 355 (2019) https://doi.org/10.1038/s41586-019-1470-2
Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet
Joanna Dra̧żkowska, Shengtai Li, Til Birnstiel, Sebastian M. Stammler and Hui Li The Astrophysical Journal 885(1) 91 (2019) https://doi.org/10.3847/1538-4357/ab46b7
The Galilean Satellites Formed Slowly from Pebbles
Yuhito Shibaike, Chris W. Ormel, Shigeru Ida, Satoshi Okuzumi and Takanori Sasaki The Astrophysical Journal 885(1) 79 (2019) https://doi.org/10.3847/1538-4357/ab46a7
Vortex instabilities triggered by low-mass planets in pebble-rich, inviscid protoplanetary discs
Migrating super-Earths in low-viscosity discs: unveiling the roles of feedback, vortices, and laminar accretion flows
Colin P McNally, Richard P Nelson, Sijme-Jan Paardekooper and Pablo Benítez-Llambay Monthly Notices of the Royal Astronomical Society 484(1) 728 (2019) https://doi.org/10.1093/mnras/stz023
Rocky super-Earths or waterworlds: the interplay of planet migration, pebble accretion, and disc evolution
Is the ring inside or outside the planet?: the effect of planet migration on dust rings
Farzana Meru, Giovanni P Rosotti, Richard A Booth, Pooneh Nazari and Cathie J Clarke Monthly Notices of the Royal Astronomical Society 482(3) 3678 (2019) https://doi.org/10.1093/mnras/sty2847
How much does turbulence change the pebble isolation mass for planet formation?