| タイトル | Infrared photometry and spectrophotometry of G75.84+0.4 |
| 著者（英） | Soifer, B. T.; Pipher, J. L.; Krassner, J. |
| 著者所属（英） | California Inst. of Tech. |
| 発行日 | 1979-05-01 |
| 言語 | eng |
| 内容記述 | Photometric mapping of G75.84+0.4 at 12.6 microns is compared with previously published radio maps of the region to deduce the relative dust/gas mass ratio for the dust responsible for the 12.6-micron emission. Spectrophotometry from 2-4 microns and 8-13 microns of the highest-emission-measure region reveals the presence of the fine structure lines of forbidden Ar III at 8.99 microns, forbidden Ne II at 12.78 microns, and forbidden S IV at 10.53 microns. Estimates of the abundance of these ions are made, and the nature of the exciting source is discussed. |
| NASA分類 | ASTRONOMY |
| レポートNO | 79A36862 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/427091 |
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