| タイトル | Molecular diagnostics of interstellar shocks |
| 著者（英） | Oppenheimer, M.; Hartquist, T. W.; Dalgarno, A. |
| 著者所属（英） | Harvard-Smithsonian Center for Astrophysics |
| 発行日 | 1980-02-15 |
| 言語 | eng |
| 内容記述 | The chemistry of molecules in shocked regions of the interstellar gas is considered and calculations are carried out for a region subjected to a shock at a velocity of 8 km/sec. Substantial enhancements are predicted in the concentrations of the molecules H2S, SO, and SiO compared to those anticipated in cold interstellar clouds. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 80A26994 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/422455 |
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