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...
| Κύριοι συγγραφείς: | , , |
|---|---|
| Μορφή: | Online |
| Γλώσσα: | spa |
| Έκδοση: |
Universidad Pedagógica y Tecnológica de Colombia
2018
|
| Θέματα: | |
| Διαθέσιμο Online: | https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812 |
