Carregant...
Dust in and near the orion nebula
Although the blister model for the Orion Nebula is widely accepted, an alternative model, where the opticalappearance of the nebula is primarily determined by self-extinction, continues to be considered by some andhas never specically been disproven. I summarize the characteristics of the two models...
Guardat en:
| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autor principal: | |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2002
|
| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57112007 |
| Etiquetes: |
Afegir etiqueta
Sense etiquetes, Sigues el primer a etiquetar aquest registre!
|