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
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2018-12-272024-07-08T14:23:57Z2024-07-08T14:23:57Zhttps://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/881210.19053/01217488.v10.n1.2019.8812https://repositorio.uptc.edu.co/handle/001/15269In 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.application/pdfspaspaUniversidad Pedagógica y Tecnológica de Colombiahttps://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812/8296Ciencia En Desarrollo; Vol. 10 No. 1 (2019): Vol 10, Núm. 1 (2019): Enero - Junio; 41-48Ciencia en Desarrollo; Vol. 10 Núm. 1 (2019): Vol 10, Núm. 1 (2019): Enero - Junio; 41-482462-76580121-7488Discos de transición, disco protoplanetario, simulación de discos protoplanetarios.Statistical model of the distribution of matter of protoplanetary disksModelo estadístico de la distribución de materia de los discos protoplanetariosinfo:eu-repo/semantics/articlehttp://purl.org/coar/version/c_970fb48d4fbd8a85http://purl.org/coar/resource_type/c_2df8fbb1http://purl.org/coar/access_right/c_abf2Poveda Tejada, NicanorRodríguez Cuevas, Luz MaryVera Villamizar, N.001/15269oai:repositorio.uptc.edu.co:001/152692025-07-18 10:56:33.112metadata.onlyhttps://repositorio.uptc.edu.coRepositorio Institucional UPTCrepositorio.uptc@uptc.edu.co |
| dc.title.en-US.fl_str_mv |
Statistical model of the distribution of matter of protoplanetary disks |
| dc.title.es-ES.fl_str_mv |
Modelo estadístico de la distribución de materia de los discos protoplanetarios |
| title |
Statistical model of the distribution of matter of protoplanetary disks |
| spellingShingle |
Statistical model of the distribution of matter of protoplanetary disks Discos de transición, disco protoplanetario, simulación de discos protoplanetarios. |
| title_short |
Statistical model of the distribution of matter of protoplanetary disks |
| 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_sort |
Statistical model of the distribution of matter of protoplanetary disks |
| dc.subject.es-ES.fl_str_mv |
Discos de transición, disco protoplanetario, simulación de discos protoplanetarios. |
| topic |
Discos de transición, disco protoplanetario, simulación de discos protoplanetarios. |
| 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. |
| publishDate |
2018 |
| dc.date.accessioned.none.fl_str_mv |
2024-07-08T14:23:57Z |
| dc.date.available.none.fl_str_mv |
2024-07-08T14:23:57Z |
| dc.date.none.fl_str_mv |
2018-12-27 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article |
| dc.type.coarversion.fl_str_mv |
http://purl.org/coar/version/c_970fb48d4fbd8a85 |
| dc.type.coar.fl_str_mv |
http://purl.org/coar/resource_type/c_2df8fbb1 |
| dc.identifier.none.fl_str_mv |
https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812 10.19053/01217488.v10.n1.2019.8812 |
| dc.identifier.uri.none.fl_str_mv |
https://repositorio.uptc.edu.co/handle/001/15269 |
| url |
https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812 https://repositorio.uptc.edu.co/handle/001/15269 |
| identifier_str_mv |
10.19053/01217488.v10.n1.2019.8812 |
| dc.language.none.fl_str_mv |
spa |
| dc.language.iso.none.fl_str_mv |
spa |
| language |
spa |
| dc.relation.none.fl_str_mv |
https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/8812/8296 |
| dc.rights.coar.fl_str_mv |
http://purl.org/coar/access_right/c_abf2 |
| rights_invalid_str_mv |
http://purl.org/coar/access_right/c_abf2 |
| dc.format.none.fl_str_mv |
application/pdf |
| dc.publisher.es-ES.fl_str_mv |
Universidad Pedagógica y Tecnológica de Colombia |
| dc.source.en-US.fl_str_mv |
Ciencia En Desarrollo; Vol. 10 No. 1 (2019): Vol 10, Núm. 1 (2019): Enero - Junio; 41-48 |
| dc.source.es-ES.fl_str_mv |
Ciencia en Desarrollo; Vol. 10 Núm. 1 (2019): Vol 10, Núm. 1 (2019): Enero - Junio; 41-48 |
| dc.source.none.fl_str_mv |
2462-7658 0121-7488 |
| institution |
Universidad Pedagógica y Tecnológica de Colombia |
| repository.name.fl_str_mv |
Repositorio Institucional UPTC |
| repository.mail.fl_str_mv |
repositorio.uptc@uptc.edu.co |
| _version_ |
1839633839254667264 |