No evidence for significant age spreads in young massive LMC clusters
ABSTRACT: Recent discoveries have put the picture of stellar clusters being simple stellar populations into question. In particular, the color magnitude diagrams of intermediate age (1–2 Gyr) massive clusters in the Large Magellanic Cloud (LMC) show features that could be interpreted as age spreads...
- Autores:
-
Silva Villa, Esteban
Niederhofer, F.
Hilker, M.
Bastian, N.
- Tipo de recurso:
- Article of investigation
- Fecha de publicación:
- 2015
- Institución:
- Universidad de Antioquia
- Repositorio:
- Repositorio UdeA
- Idioma:
- eng
- OAI Identifier:
- oai:bibliotecadigital.udea.edu.co:10495/32712
- Acceso en línea:
- https://hdl.handle.net/10495/32712
- Palabra clave:
- Galaxias
Galaxies
Estrellas
Stars
Estrellas - evolución
Stars - evolution
Magellanic Clouds
Diagrama de Hertzsprung-Russell
- Rights
- openAccess
- License
- http://creativecommons.org/licenses/by/2.5/co/