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Planetary nebulae with double shells and haloes: insights from hydrodynamical simulations
We combined hydrodynamical simulations with stellar evolutionary calculations based on prescribed mass-lossrates in order to get a better understanding of how structure and kinematics of circumstellar matter developwith time during the late AGB and the following post-AGB and Planetary Nebula (PN) ev...
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| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
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| Main Authors: | , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2002
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| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57112048 |
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