| タイトル | The emission/absorption FE 2 spectrum of HD 45677 |
| 本文（外部サイト） | http://hdl.handle.net/2060/19810017382 |
| 著者（英） | Stalio, R.; Selvelli, P. L. |
| 著者所属（英） | Osservatorio Astronomico |
| 発行日 | 1981-01-01 |
| 言語 | eng |
| 内容記述 | The complex behavior of the emission/absorption spectrum of Fe II is analyzed. The far UV spectrum is characterized almost solely by absorption lines, while, in the near UV, strong emissions are predominant. Radiative excitation from the ground to the highest levels (chi is approximately 10 eV) with re-emission in the near UV, visible and I.R. seems to be the main mechanism capable of explaining the observed spectral features. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 81N25918 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/568161 |
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