Detalhes bibliográficos
| Ano de defesa: |
2022 |
| Autor(a) principal: |
Souza, Jefferson Wherculis da Silva |
| Orientador(a): |
Não Informado pela instituição |
| Banca de defesa: |
Não Informado pela instituição |
| Tipo de documento: |
Dissertação
|
| Tipo de acesso: |
Acesso aberto |
| Idioma: |
por |
| Instituição de defesa: |
Não Informado pela instituição
|
| Programa de Pós-Graduação: |
Não Informado pela instituição
|
| Departamento: |
Não Informado pela instituição
|
| País: |
Não Informado pela instituição
|
| Palavras-chave em Português: |
|
| Link de acesso: |
http://www.repositorio.ufc.br/handle/riufc/64394
|
Resumo: |
Using a generalized function of the stellar spin-down law, we investigate the dependence of the magnetic braking index on the age of different clusters. Initially, our research consists of 14 open clusters with age less than 1 Gigayear and ranging in mass from 0.7 to 1.4 $M_{\odot}$ distributed in three subsamples. We also used $6$ open clusters and $1$ globular cluster with ages greater than 1 Gigayear. Our objective is to verify the temporal behavior of the non-extensive braking index $q$ which brings the cumulative distribution of the rotational velocities of the stars of the youngest cluster $X$ taken at the future age of an older cluster denoted by $Y$. As a result, the $q$ -index is calculated over time $t_{Y}-t_{X}$, where $t_{Y}$ denotes the age of the oldest open cluster used to estimate the future cumulative distribution of the rotation velocity of the cluster $X$ with the current age $t_{X}$. Our results indicate that for clusters younger than $1$ Gigayear, the values of $q$ are slightly constant. For clusters older than $1$ Gigayear, the results found for the temporal evolution of the magnetic brake index also showed a smoothly constant behavior for the values of $q$. The results also indicate a decrease in stellar rotation caused by the deceleration of the magnetic brake index. |
