Using planetary nebulae to probe the structure of the galactic thin disk
Most planetary nebulae appear to arise from progenitors with mass MPG 1 M. One would therefore expect them to be closely associated with stars locatedwithin the galactic thin disk. This has been confrmed through a series of recentestimates of scale height, which imply values z0(PNe) of order 220 pc...
Guardat en:
| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autor principal: | |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2005
|
| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57141205 |
| Etiquetes: |
Sense etiquetes, Sigues el primer a etiquetar aquest registre!
|