Por favor, use este identificador para citar o enlazar este ítem: http://cybertesis.uni.edu.pe/handle/uni/553
Título : Estabilidad dinámica de estrellas axisimétricas
Autor : Vidalón Vidalón, Edgard
Asesor : Bernui Leo, Armando
Palabras clave : Dinámica;Estrellas Axisimétricas
Fecha de publicación : 2003
Editorial : Universidad Nacional de Ingeniería
Resumen : Here we study the dynamics of rotation of Newtonian fluid ellipsoids, specifically its stability proper¬ties. We use this approach to model star condensation from an original homogeneous gas cloud, in order to understand the Sun’s evolution from a primitive gas nebula to became a hot star. Finally we apply our results to a more realistic pre-solar model, considering the nebula formed by two different -but homogeneous- axially symmetric gas clouds, one being a nucleus and the other being a shell covering the nucleus. The results are very interesting and match very well with the present knowledge about the formation of our solar system. This suggest that, with further work, this model could be used to improve our understanding of planetary-star formation processes.
URI : http://cybertesis.uni.edu.pe/handle/uni/553
Derechos: info:eu-repo/semantics/openAccess
Aparece en las colecciones: Maestría

Ficheros en este ítem:
Fichero Descripción Tamaño Formato  
vidalon_ve.pdf88,28 MBAdobe PDFVisualizar/Abrir

Este ítem está sujeto a una licencia Creative Commons Licencia Creative Commons Creative Commons