Luminous Stars in Nearby Galaxies
Studies on the populations of luminous stars in nearby resolved galaxies have revealed a complex distribution in the luminosity–temperature plane (the HR diagram). The fundamentals of massive star evolution are mostly understood, but the roles of mass loss, episodic mass loss, rotation, and binarity...
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Formato: | Libro electrónico |
Idioma: | Inglés |
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Basel, Switzerland
MDPI - Multidisciplinary Digital Publishing Institute
2020
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Ver en Biblioteca Universitat Ramon Llull: | https://discovery.url.edu/permalink/34CSUC_URL/1im36ta/alma991009654108106719 |