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...
Salvato in:
| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autore principale: | |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2002
|
| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57112007 |
| Tags: |
Nessun Tag, puoi essere il primo ad aggiungerne!!
|