日本地球惑星科学連合2019年大会

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[J] 口頭発表

セッション記号 P (宇宙惑星科学) » P-CG 宇宙惑星科学複合領域・一般

[P-CG24] アルマによる惑星科学の新展開

2019年5月29日(水) 10:45 〜 12:15 105 (1F)

コンビーナ:武藤 恭之(工学院大学 教育推進機構)、百瀬 宗武(茨城大学理学部)、佐川 英夫(京都産業大学理学部)、下条 圭美(国立天文台)、座長:百瀬 宗武(茨城大学)

11:30 〜 11:45

[PCG24-09] The Synthetic ALMA Multiband Analysis of the Dust Properties of the TW Hya Protoplanetary Disk

*Seongjoong Kim1Hideko Nomura1Takashi Tsukagoshi2Ryohei Kawabe2,3,4Takayuki Muto5 (1.Department of Earth and Planetary Sciences, Tokyo Institute of Technology、2.National Astronomical Observatory of Japan、3.The Graduate University for Advanced Studies (SOKENDAI)、4.Department of Astronomy, School of Science, University of Tokyo、5.Division of Liberal Arts, Kogakuin University)

キーワード:methods: observational, protoplanetary disks, stars: individual (TW Hydrae)

Analyzing multiband observations of dust continuum emission is one of the useful tools to constrain dust properties which help us to understand the physical properties of the disks. We perform the synthetic ALMA multiband analysis to find the best ALMA band set for constraining the dust properties of the TW Hya protoplanetary disk. We find that the Band [10,6,3] set is the best set among the possible combinations of ALMA Band [3,4,5,6,7,8,9,10]. We also find two conditions for the good ALMA band sets providing narrow constraint ranges on dust properties; (1) Band 9 or 10 is included in the band set and (2) Enough frequency intervals between the bands. These are related with the conditions which give good constraints on dust properties: the combination of optically thick and thin bands are required, and large β (β is the power-law index of dust opacity, κν ∝ νβ) and low dust temperature are preferable. To examine our synthetic analysis results, we apply the multiband analysis to ALMA archival data of the TW Hya disk at Band 4, 6, 7, and 9. Band [9,6,4] set provides the dust properties close to the model profile, while Band [7,6,4] set gives the dust properties deviating from the model at all radii with too broad constraint range to specify the accurate values of dust temperature, optical depth, and β. Since these features are expected by the synthetic multiband analysis, we confirm that the synthetic multiband analysis is well consistent with the results derived from real data.