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most citedRapid Coagulation of Porous Dust Aggregates Outside the Snow Line: A Pathway to Successful Icy Planetesimal Formation

435 citations · 3k across the 62 of their papers we have counts for

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Showing 2013Show all

5 papers · 1 filter

astro-ph.EP2013★ 30 cited

Crowding Out of Giants by Dwarfs: An Origin for the Lack of Companion Planets in Hot Jupiter Systems

Masahiro Ogihara, Shu-ichiro Inutsuka, Hiroshi Kobayashi

We investigate formation of close-in terrestrial planets from planetary embryos under the influence of a hot Jupiter (HJ) using gravitational N-body simulations that include gravit…

astro-ph.SR2013★ 154 cited

Local Enhancement of Surface Density in the Protoplanetary Ring Surrounding HD 142527

Misato Fukagawa, Takashi Tsukagoshi, Munetake Momose +15

We report ALMA observations of dust continuum, 13CO J=3--2, and C18O J=3--2 line emission toward a gapped protoplanetary disk around HD 142527. The outer horseshoe-shaped disk show…

astro-ph.EP2013★ 86 cited

Condition for Capture into First-order Mean Motion Resonances and Application to Constraints on Origin of Resonant Systems

Masahiro Ogihara, Hiroshi Kobayashi

We investigate the condition for capture into first-order mean motion resonances using numerical simulations with a wide range of various parameters. In particular, we focus on der…

astro-ph.EP2013★ 49 cited

Small Planetesimals in a Massive Disk Formed Mars

Hiroshi Kobayashi, Nicolas Dauphas

Mars is likely to be a planetary embryo formed through collisions with planetesimals, which can explain its small mass and rapid formation timescale obtained from 182Hf-182$W chron…

astro-ph.GA2013★ 26 cited

Evolution of dust grain size distribution by shattering in the interstellar medium: robustness and uncertainty

Hiroyuki Hirashita, Hiroshi Kobayashi

Shattering of dust grains in the interstellar medium is a viable mechanism of small grain production in galaxies. We examine the robustness or uncertainty in the theoretical predic…