Statistical model of the distribution of matter of protoplanetary disks

In the majority of models, the protoplanetary disks have a continuous distribution of gas and dust, with a dynamics that gives origin to the planets, which in the process of formation, make grooves on the disk by gravitationally capturing the existing matter around them. Transition disks are a cl...

詳細記述

書誌詳細
主要な著者: Poveda Tejada, Nicanor, Rodríguez Cuevas, Luz Mary, Vera Villamizar, N.
フォーマット: Online
言語:spa
出版事項: Universidad Pedagógica y Tecnológica de Colombia 2018
主題:
オンライン・アクセス:https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812

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