Formation of Transition Alumina Dust around Asymptotic Giant Branch Stars: Condensation Experiments using Induction Thermal Plasma Systems

1,2Aki Takigawa,3Tae-Hee Kim,4Yohei Igami,2Tatsuki Umemoto,2,7Akira Tsuchiyama,5Chiyoe Koike,2Junya Matsuno,6Takayuki Watanabe
The Astrophysical Journal Letters, 878, L7 Link to Article [DOI
https://doi.org/10.3847/2041-8213/ab1f80]
1The Hakubi Center for Advanced Research, Kyoto University, Kitashirakawa-Oiwakecho, Sakyo, Kyoto 606-8502, Japan
2Division of Earth and Planetary Sciences, Kyoto University, Kitashirakawa-Oiwakecho, Sakyo, Kyoto 606-8502, Japan
3Institute for Nuclear Science and Technology, Department of Nuclear and Energy Engineering, Jeju National University, 102 Jejudaehak-ro, Jeju-si, Jeju, 63243, Republic of Korea
4Institute of Materials and Systems for Sustainability, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8603, Japan
5Department of Physics, Ritsumeikan University, 1-1-1 Nojihigashi, Kusatsu-shi, Shiga 525-8577, Japan
6Department of Chemical Engineering, Kyushu University, Fukuoka 819-0395, Japan
7Present addresses: Research Organization of Science and Technology, Ritsumeikan University, 1-1-1 Nojihigashi, Kusatsu, Shiga 525-8577, Japan, and Guangzhou Institute of Geochemistry, Chinese Academy of Sciences 511 Kehua Street, Wushan, Tianhe District, Guangzhou, 510640, China.

 

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