Constraints on type ia supernovae from near infrared spectra
We describe a research program to improve the understanding of Type IaSupernovae (SNe Ia) by modeling and observing near infrared (NIR) spectra ofthese events. The NIR between 0.9 and 2.5 is optimal for examining certainproducts of the SNe Ia explosion that may be blended or obscured in other spectr...
Gespeichert in:
| Veröffentlicht in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hauptverfasser: | , , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
Universidad Nacional Autónoma de México
2001
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| Schlagworte: | |
| Online-Zugang: | https://www.redalyc.org/articulo.oa?id=57101042 |
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