Research theme for competitive and other funds (3):
2019 - 2021 微小ダストの磁場整列で解き明かす円盤のミリ波偏波の起源
2017 - 2020 最新ダスト光学モデルに基づく微惑星形成理論の観測的検証
2016 - 2019 Modeling the coevolution of dust and the snow line in protoplanetary disks
Papers (26):
Hidekazu Tanaka, Ryoichi Anayama, Ryo Tazaki. Compression of Dust Aggregates via Sequential Collisions with High Mass Ratios. ASTROPHYSICAL JOURNAL. 2023. 945. 1
Mitsuhiko Honda, Ryo Tazaki, Koji Murakawa, Hiroshi Terada, Tomoyuki Kudo, Takashi Hattori, Jun Hashimoto, Motohide Tamura, Makoto Watanabe. Subaru/IRCS L-band spectro-polarimetry of the HD 142527 disk scattered light. Publications of the Astronomical Society of Japan. 2022. 74. 4. 851-856
Kazumasa Ohno, Xi Zhang, Ryo Tazaki, Satoshi Okuzumi. Haze Formation on Triton. The Astrophysical Journal. 2021. 912. 1. 37-37
Ryo Tazaki, Koji Murakawa, Takayuki Muto, Mitsuhiko Honda, Akio K. Inoue. Scattering Polarization of 3 mu m Water-ice Feature by Large Icy Grains. ASTROPHYSICAL JOURNAL. 2021. 910. 1
Taichi Uyama, Thayne Currie, Valentin Christiaens, Jaehan Bae, Takayuki Muto, Sanemichi Z. Takahashi, Ryo Tazaki, Marie Ygouf, Jeremy N. Kasdin, Tyler Groff, et al. SCExAO/CHARIS High-contrast Imaging of Spirals and Darkening Features in the HD 34700 A Protoplanetary Disk. The Astrophysical Journal. 2020. 900. 2. 135-135