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Enhanced mass loss rates in red supergiants and their impact on the circumstellar medium

In this work, we present models of massive stars between 15 and 23 M⊙, with enhanced mass loss rates during the red supergiant phase. Our aim is to explore the impact of extreme red supergiant mass-loss on stellar evolution and on their circumstellar medium. We computed a set of numerical experiment...

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Vydáno v:Revista Mexicana de Astronomía y Astrofísica
Hlavní autoři: L. Hernández-Cervantes, B. Pérez-Rendón, A. Santillán, G. García-Segura, C. Rodríguez-Ibarra
Médium: Artigo
Jazyk:Inglês
Vydáno: Universidad Nacional Autónoma de México 2019
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On-line přístup:https://www.redalyc.org/articulo.oa?id=57171631004
https://www.redalyc.org/journal/571/57171631004/
https://www.redalyc.org/journal/571/57171631004/html/
https://www.redalyc.org/journal/571/57171631004/57171631004.epub
https://www.redalyc.org/journal/571/57171631004/movil
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