| タイトル | Discovery of high-ionization far-ultraviolet line emission from the interstellar medium |
| 著者（英） | Bowyer, Stuart; Martin, Christopher |
| 著者所属（英） | California Univ. |
| 発行日 | 1990-02-10 |
| 言語 | eng |
| 内容記述 | Diffuse, highly ionized line emission from the 1550 lines of C IV and the 1663 lines of O II was discovered on Space Shuttle mission 61-C. The emission-lines ratios are consistent with a single temperature in most directions, although there is some evidence that the emission results from gas with a nonequilibrium ionization balance and a distribution of temperatures. It is concluded that the observation of UV emission is consistent only with a galactic fountain model with a fountain having a mass flux of 6-25 solar mass/yr and a luminosity of (2.5-13) X 10 to the 40th ergs/s. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 90A24894 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/358066 |
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