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Mitsuhiko Honda

Researcher at Kurume University

Publications -  95
Citations -  3846

Mitsuhiko Honda is an academic researcher from Kurume University. The author has contributed to research in topics: Protoplanetary disk & Spectral energy distribution. The author has an hindex of 30, co-authored 93 publications receiving 3611 citations. Previous affiliations of Mitsuhiko Honda include Kanagawa University & Subaru.

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Discovery of Small-Scale Spiral Structures in the Disk of SAO 206462 (HD 135344B): Implications for the Physical State of the Disk from Spiral Density Wave Theory

Takayuki Muto, +69 more
TL;DR: In this article, high-resolution, H-band, imaging observations, collected with Subaru/HiCIAO, of the scattered light from the transitional disk around SAO 206462 (HD 135344B), reveal the presence of scattered light components as close as 0.2 (approx 28 AU).
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Direct Imaging of Fine Structures in Giant Planet Forming Regions of the Protoplanetary Disk around AB Aurigae

TL;DR: In this article, high-resolution 1.6 μm polarized intensity (PI) images of the circumstellar disk around the Herbig Ae star AB Aur at a radial distance of 22 AU (015) up to 554 AU (385) were obtained by the high-contrast instrument HiCIAO with the dual-beam polarimetry.
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Local Enhancement of Surface Density in the Protoplanetary Ring Surrounding HD 142527

TL;DR: In this article, the surface density of the outer horseshoe-shaped disk was estimated from the optically thick 13CO J=3--2 emission. And the lower limit of the peak surface density was calculated to be 28 g cm-2 by assuming a canonical gas-to-dust mass ratio of 100.
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Polarimetric Imaging of Large Cavity Structures in the Pre-transitional Protoplanetary Disk around PDS 70: Observations of the Disk

Jun Hashimoto, +58 more
TL;DR: In this paper, high-resolution H-band polarized intensity (PI; FWHM = 0."1: 14 AU) and L'-band imaging data (FWHM= 0."11: 15 AU) of the circumstellar disk around the weak-lined T Tauri star PDS 70 in Centaurus at a radial distance of 28 AU (0."2) up to 210 AU (1."5).