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 class...
- Autores:
- Tipo de recurso:
- Fecha de publicación:
- 2018
- Institución:
- Universidad Pedagógica y Tecnológica de Colombia
- Repositorio:
- RiUPTC: Repositorio Institucional UPTC
- Idioma:
- spa
- OAI Identifier:
- oai:repositorio.uptc.edu.co:001/15269
- Acceso en línea:
- https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812
https://repositorio.uptc.edu.co/handle/001/15269
- Palabra clave:
- Discos de transición, disco protoplanetario, simulación de discos protoplanetarios.
- Rights
- License
- http://purl.org/coar/access_right/c_abf2