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 (25)：
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
Ryo Kandori, Motohide Tamura, Masao Saito, Kohji Tomisaka, Tomoaki Matsumoto, Ryo Tazaki, Tetsuya Nagata, Nobuhiko Kusakabe, Yasushi Nakajima, Jungmi Kwon, et al. Distortion of Magnetic Fields in the Dense Core SL 42 (CrA-E) in the Corona Australis Molecular Cloud Complex. The Astrophysical Journal. 2020. 900. 1. 20-20
