932 citations · 3.3k across the 35 of their papers we have counts for
35 papers
Similar-mass versus diverse-mass planetary systems in wind-driven accretion discs
Yunpeng Zhao, Soko Matsumura
Many close-in multiple-planet systems show a peas-in-a-pod trend, where neighbouring planets have similar sizes, masses, and orbital spacing. Others, including the Solar System, ha…
Giant planet formation in the solar system
Anuja Raorane, Ramon Brasser, Soko Matsumura +3
The formation history of Jupiter has been of interest due to its ability to shape the solar system's history. Yet little attention has been paid to the formation and growth of Satu…
Can the giant planets of the Solar System form via pebble accretion in a smooth protoplanetary disc?
Tommy Chi Ho Lau, Man Hoi Lee, Ramon Brasser +1
Prevailing -body planet formation models typically start with lunar-mass embryos and show a general trend of rapid migration of massive planetary cores to the inner Solar System…
The STAR-MELT Python package for emission line analysis of YSOs
Justyn Campbell-White, Aurora Sicilia-Aguilar, Carlo F. Manara +4
We introduce the STAR-MELT Python package that we developed to facilitate the analysis of time-resolved emission line spectroscopy of young stellar objects. STAR-MELT automatically…
N-body simulations of planet formation via pebble accretion II. How various giant planets form
Soko Matsumura, Ramon Brasser, Shigeru Ida
Aims. The connection between initial disc conditions and final orbital and physical properties of planets is not well-understood. In this paper, we numerically study the formation…
A new and simple prescription for planet orbital migration and eccentricity damping by planet-disc interactions based on dynamical friction
Shigeru Ida, Takayuki Muto, Soko Matsumura +1
During planet formation gravitational interaction between a planetary embryo and the protoplanetary gas disc causes orbital migration of the planetary embryo, which plays an import…