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...
| المؤلفون الرئيسيون: | , , |
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| التنسيق: | Online |
| اللغة: | spa |
| منشور في: |
Universidad Pedagógica y Tecnológica de Colombia
2018
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| الموضوعات: | |
| الوصول للمادة أونلاين: | https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812 |
