Carregant...
Coronal physics and the chandra emission line project
With the launch of the Chandra X-ray Observatory, high resolution X-rayspectroscopy of cosmic sources has begun. Early, deep observations of three stellarcoronal sources|Capella, Procyon, and HR 1099|are providing not only invaluablecalibration data, but also benchmarks for plasma spectral models. T...
Guardat en:
| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2000
|
| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57100907 |
| Etiquetes: |
Afegir etiqueta
Sense etiquetes, Sigues el primer a etiquetar aquest registre!
|