S
Soko Matsumura
Researcher at University of Dundee
Publications - 64
Citations - 4227
Soko Matsumura is an academic researcher from University of Dundee. The author has contributed to research in topics: Planet & Planetary system. The author has an hindex of 33, co-authored 64 publications receiving 3946 citations. Previous affiliations of Soko Matsumura include McMaster University & University of Maryland, College Park.
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Journal ArticleDOI
Dynamical Outcomes of Planet-Planet Scattering
TL;DR: In this article, the initial planetary masses and orbits of three giant planets with and without residual gas disks were assigned in a realistic manner following the core accretion model of planet formation.
Journal ArticleDOI
A COMBINED SUBARU/VLT/MMT 1-5 μm STUDY OF PLANETS ORBITING HR 8799: IMPLICATIONS FOR ATMOSPHERIC PROPERTIES, MASSES, AND FORMATION
Thayne Currie,Adam Burrows,Yoichi Itoh,Soko Matsumura,Misato Fukagawa,Daniel Apai,Nikku Madhusudhan,Philip M. Hinz,Timothy J. Rodigas,Markus Kasper,Tae-Soo Pyo,Satoshi Ogino +11 more
TL;DR: In this article, the authors presented new 1-1.25 micron (z and J band) Subaru/IRCS and 2-3 micron VLT/NaCo data for HR 8799 and a rereduction of the 3-5 micron MMT/Clio data first presented by Hinz et al.
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A Combined Subaru/VLT/MMT 1--5 Micron Study of Planets Orbiting HR 8799: Implications for Atmospheric Properties, Masses, and Formation
Thayne Currie,Adam Burrows,Yoichi Itoh,Soko Matsumura,Misato Fukagawa,Daniel Apai,Nikku Madhusudhan,Phil Hinz,Timothy J. Rodigas,Markus Kasper,Tae-Soo Pyo,Satoshi Ogino +11 more
TL;DR: In this paper, the authors presented new 1.25 micron (z and J band) Subaru/IRCS and 2-micron (K band) VLT/NaCo data for HR 8799 and a rereduction of the 3-5 micron MMT/Clio data first presented by Hinz et al.
Journal ArticleDOI
Tidal evolution of close-in planets
TL;DR: In this article, the authors investigate the evolution of transiting planets on eccentric orbits, and find that there are two characteristic evolution paths for them, depending on the relative efficiency of tidal dissipation inside the star and the planet.
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Gas disks to gas giants: simulating the birth of planetary systems.
TL;DR: In this article, the authors present self-consistent numerical simulations of the process of converting a protostellar disk into a small number of planetary bodies, which produce results in agreement with some of the key trends observed in the properties of exoplanets.