Dusty super star cluster winds: their impact on the interstellar medium and infrared manifestations
In light of the growing evidence pointing at core-collapse supernovae as large dust producers, and given their immense number in young massive stellar clusters (SSCs), this work is devoted to address the influence of stochastic injection, sputtering and outflow of dust grains on their emission prope...
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| Formato: | tesis doctoral |
| Estado: | Versión publicada |
| Fecha de publicación: | 2015 |
| País: | México |
| Recursos: | Instituto Nacional de Astrofísica, Óptica y Electrónica |
| Repositorio: | Repositorio Institucional del INAOE |
| Idioma: | inglés |
| OAI Identifier: | oai:inaoe.repositorioinstitucional.mx:1009/19 |
| Acesso em linha: | http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/19 |
| Access Level: | acceso abierto |
| Palavra-chave: | info:eu-repo/classification/Hidrodinámica/Hydrodinamics info:eu-repo/classification/Estrella/Star clusters info:eu-repo/classification/Estelar/Stellar winds info:eu-repo/classification/Polvo cósmico/Cosmic dust info:eu-repo/classification/Medio/Interstellar medium info:eu-repo/classification/cti/1 info:eu-repo/classification/cti/21 info:eu-repo/classification/cti/2105 |
| Resumo: | In light of the growing evidence pointing at core-collapse supernovae as large dust producers, and given their immense number in young massive stellar clusters (SSCs), this work is devoted to address the influence of stochastic injection, sputtering and outflow of dust grains on their emission properties inside the hot and dense intracluster medium. The theory of dust radiative cooling, which considers time-dependent dust size distributions and chemical composition, is combined with a self-consistent semi-analytic method, in order to study the hydrodynamics of spherically symmetric winds driven by SSCs with a generalized Schuster stellar density profile. |
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