Dust particles on a photon diet in V605 AQl
We present a new model to explain the excess in mid and near infrared emission of V605 Aql. This hydrogenpoor object is of special interest because it formed after a late helium ash of the central star in the planetarynebula Abell 58. Simple grain size models with an equilibrium dust temperature can...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autore principale: | |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2002
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| Accesso online: | https://www.redalyc.org/articulo.oa?id=57112063 |
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