Formation of Protostellar Clusters’ Computational Model: an application to ‘the Brick’.
In the present work, we show results of a numerical simulation project aimed to study the formation process of the interstellar cloud known as “the Brick”. This cloud is located near the Milky Way center. The simulated formation process is based on the collision of two gas sub-clouds that are contai...
שמור ב:
| מחבר ראשי: | |
|---|---|
| פורמט: | Online |
| שפה: | spa |
| יצא לאור: |
Universida de Sonora
2022
|
| גישה מקוונת: | https://epistemus.unison.mx/index.php/epistemus/article/view/225 |
| תגים: |
הוספת תג
אין תגיות, היה/י הראשונ/ה לתייג את הרשומה!
|
| id |
oai:http:--epistemus.unison.mx:article-225 |
|---|---|
| record_format |
ojs |
| spelling |
oai:http:--epistemus.unison.mx:article-2252023-06-14T01:03:10Z Formation of Protostellar Clusters’ Computational Model: an application to ‘the Brick’. Modelo computacional de la formación de cúmulos proto-estelares: aplicación a “the Brick” Arreaga Garcia, Guillermo astrophysics computation simulations protostars astrofisica computacion simulaciones protoestrellas In the present work, we show results of a numerical simulation project aimed to study the formation process of the interstellar cloud known as “the Brick”. This cloud is located near the Milky Way center. The simulated formation process is based on the collision of two gas sub-clouds that are contained within a larger progenitor cloud. A fundamental characteristic is that the simulated gas shows turbulent velocities. The results of several simulations that well represent some cases of academic interest are studied besides the case of the cloud “the Brick”. In addition, we calculate the physical properties of the groups of proto- star resulting from such models. Due to the obtained mass, these groups can be identified as protostellar clusters. En el presente trabajo se exponen los resultados de un proyecto de simulación numérica diseñado para estudiar el proceso de formación de la nube interestelar conocida como "the Brick". Dicha nube está localizada cerca del centro de la Vía Láctea. El proceso de formación simulado está basado en la colisión de dos sub-nubes de gas que están contenidas en una nube progenitora mayor. Una característica fundamental es que el gas que simulamos muestra velocidades turbulentas. Estudiamos los resultados de varias simulaciones que representan bien algunos casos de interés académico, además del caso de la nube “the Brick”. Adicionalmente, calculamos las propiedades físicas de los grupos de proto-estrellas resultantes de tales modelos. Por la masa obtenida, dichos grupos se pueden identificar como cúmulos proto-estelares. Universida de Sonora 2022-11-24 info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Academy Academia application/pdf application/pdf text/xml https://epistemus.unison.mx/index.php/epistemus/article/view/225 10.36790/epistemus.v16i33.225 EPISTEMUS; Vol. 16 No. 33 (2022): Issue 33; 39-45 EPISTEMUS; Vol. 16 Núm. 33 (2022): Revista No. 33; 39-45 2007-8196 2007-4530 spa https://epistemus.unison.mx/index.php/epistemus/article/view/225/268 https://epistemus.unison.mx/index.php/epistemus/article/view/225/310 https://epistemus.unison.mx/index.php/epistemus/article/view/225/326 Derechos de autor 2022 EPISTEMUS https://creativecommons.org/licenses/by-nc-sa/4.0 |
| institution |
Epistemus |
| collection |
OJS |
| language |
spa |
| format |
Online |
| author |
Arreaga Garcia, Guillermo |
| spellingShingle |
Arreaga Garcia, Guillermo Formation of Protostellar Clusters’ Computational Model: an application to ‘the Brick’. |
| author_facet |
Arreaga Garcia, Guillermo |
| author_sort |
Arreaga Garcia, Guillermo |
| title |
Formation of Protostellar Clusters’ Computational Model: an application to ‘the Brick’. |
| title_short |
Formation of Protostellar Clusters’ Computational Model: an application to ‘the Brick’. |
| title_full |
Formation of Protostellar Clusters’ Computational Model: an application to ‘the Brick’. |
| title_fullStr |
Formation of Protostellar Clusters’ Computational Model: an application to ‘the Brick’. |
| title_full_unstemmed |
Formation of Protostellar Clusters’ Computational Model: an application to ‘the Brick’. |
| title_sort |
formation of protostellar clusters’ computational model: an application to ‘the brick’. |
| description |
In the present work, we show results of a numerical simulation project aimed to study the formation process of the interstellar cloud known as “the Brick”. This cloud is located near the Milky Way center. The simulated formation process is based on the collision of two gas sub-clouds that are contained within a larger progenitor cloud. A fundamental characteristic is that the simulated gas shows turbulent velocities. The results of several simulations that well represent some cases of academic interest are studied besides the case of the cloud “the Brick”. In addition, we calculate the physical properties of the groups of proto- star resulting from such models. Due to the obtained mass, these groups can be identified as protostellar clusters. |
| publisher |
Universida de Sonora |
| publishDate |
2022 |
| url |
https://epistemus.unison.mx/index.php/epistemus/article/view/225 |
| work_keys_str_mv |
AT arreagagarciaguillermo formationofprotostellarclusterscomputationalmodelanapplicationtothebrick AT arreagagarciaguillermo modelocomputacionaldelaformaciondecumulosprotoestelaresaplicacionathebrick |
| _version_ |
1781317651690160128 |
