| タイトル | High-resolution X-ray observations of the Orion Nebula |
| 著者（英） | Righini-Cohen, G.; Simon, M.; Ku, W. H.-M. |
| 著者所属（英） | Columbia Univ.|State Univ. of New York |
| 発行日 | 1982-01-01 |
| 言語 | eng |
| 内容記述 | Observations of the Trapezium region in the Orion Nebula have been obtained with the high-resolution X-ray imaging instrument on the Einstein Observatory. At least 58 sources of the X-ray emission have been revealed, and all but two can be identified with visible stars. The strongest source is the star theta(1)C, which excites the emission nebula, and has an X-ray luminosity of 6 x 10 to the 32nd ergs/s. No strong X-ray emission has been observed from members of the infrared cluster embedded within the Orion molecular cloud. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 82A17698 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/412613 |
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