Massive Protostellar Disks as a Hot Laboratory of Silicate Grain Evolution

Typical accretion disks around massive protostars are hot enough for water ice to sublimate. We here propose to utilize the massive protostellar disks for investigating the collisional evolution of silicate grains with no ice mantle, which is an essential process for the formation of rocky planetesi...

詳細記述

書誌詳細
主要な著者: Ryota Yamamuro, Kei E. I. Tanaka, Satoshi Okuzumi
フォーマット: 論文
言語:English
出版事項: IOP Publishing 2023-01-01
シリーズ:The Astrophysical Journal
主題:
オンライン・アクセス:https://doi.org/10.3847/1538-4357/acc52f