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...
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| Format: | Online |
| Language: | spa |
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Universidad Pedagógica y Tecnológica de Colombia
2018
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| Online Access: | https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812 |
| _version_ | 1801706344713027584 |
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| author | Poveda Tejada, Nicanor Rodríguez Cuevas, Luz Mary Vera Villamizar, N. |
| author_facet | Poveda Tejada, Nicanor Rodríguez Cuevas, Luz Mary Vera Villamizar, N. |
| author_sort | Poveda Tejada, Nicanor |
| collection | OJS |
| description |
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 of protoplanetary disk that has a large cavity free of gas and dust inside. In this paper a statistical model based on transitional discs is proposed, which extends to protoplanetary disks. With this model you can perform dynamic simulations of planetary formation using few parameters. The process followed to simulate the transition disk DoAr44 and the protoplanetary disk Hl-Tauri is shown. Unlike other models, the formation of planetary bodies is faster.
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| format | Online |
| id | oai:oai.revistas.uptc.edu.co:article-8812 |
| institution | Revista Ciencia en Desarrollo |
| language | spa |
| publishDate | 2018 |
| publisher | Universidad Pedagógica y Tecnológica de Colombia |
| record_format | ojs |
| spelling | oai:oai.revistas.uptc.edu.co:article-88122020-11-11T02:07:04Z Statistical model of the distribution of matter of protoplanetary disks Modelo estadístico de la distribución de materia de los discos protoplanetarios Poveda Tejada, Nicanor Rodríguez Cuevas, Luz Mary Vera Villamizar, N. Discos de transición, disco protoplanetario, simulación de discos protoplanetarios. 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 of protoplanetary disk that has a large cavity free of gas and dust inside. In this paper a statistical model based on transitional discs is proposed, which extends to protoplanetary disks. With this model you can perform dynamic simulations of planetary formation using few parameters. The process followed to simulate the transition disk DoAr44 and the protoplanetary disk Hl-Tauri is shown. Unlike other models, the formation of planetary bodies is faster. En la mayoría de modelos de discos protoplanetarios se tiene una distribución continua de gas y polvo, con una dinámica que da origen a los planetas, los cuales en el proceso de formación, hacen surcos en el disco al capturar gravitacionalmente la materia existente a su alrededor. Los discos de transición son una clase de disco protoplanetario que se caracterizan por tener una gran cavidad libre de gas y polvo en su interior. En este artículo se propone un modelo estadístico basado en los discos de transición, el cual se extiende a los discos protoplanetarios. Con este modelo se pueden realizar simulaciones dinámicas de formación planetaria usando pocos parámetros. Se muestra el proceso seguido para simular el disco de transición DoAr44 y el disco protoplanetario Hl-Tauri. A diferencia de otros modelos, la formación de cuerpos planetarios es más rápida. Universidad Pedagógica y Tecnológica de Colombia 2018-12-27 info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion application/pdf https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812 10.19053/01217488.v10.n1.2019.8812 Ciencia En Desarrollo; Vol. 10 No. 1 (2019): Vol 10, Núm. 1 (2019): Enero - Junio; 41-48 Ciencia en Desarrollo; Vol. 10 Núm. 1 (2019): Vol 10, Núm. 1 (2019): Enero - Junio; 41-48 2462-7658 0121-7488 spa https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812/8296 |
| spellingShingle | Discos de transición, disco protoplanetario, simulación de discos protoplanetarios. Poveda Tejada, Nicanor Rodríguez Cuevas, Luz Mary Vera Villamizar, N. Statistical model of the distribution of matter of protoplanetary disks |
| title | Statistical model of the distribution of matter of protoplanetary disks |
| title_alt | Modelo estadístico de la distribución de materia de los discos protoplanetarios |
| title_full | Statistical model of the distribution of matter of protoplanetary disks |
| title_fullStr | Statistical model of the distribution of matter of protoplanetary disks |
| title_full_unstemmed | Statistical model of the distribution of matter of protoplanetary disks |
| title_short | Statistical model of the distribution of matter of protoplanetary disks |
| title_sort | statistical model of the distribution of matter of protoplanetary disks |
| topic | Discos de transición, disco protoplanetario, simulación de discos protoplanetarios. |
| topic_facet | Discos de transición, disco protoplanetario, simulación de discos protoplanetarios. |
| url | https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812 |
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