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Error estimates for emission lines in the hydrogen and helium isosequences
Emission lines from hydrogen and helium isosequence are among the strongestin X-ray spectra; they will soon be used to measure the temperature, density, andequilibrium state of collisionally excited, astrophysical plasmas. We have createda new plasma code, APEC, which calculates the emission from su...
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| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2000
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57100933 |
| タグ: |
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