| タイトル | HEAO 3 upper limits to the expected 1634 KeV line from SS 483 |
| 本文（外部サイト） | http://hdl.handle.net/2060/19850025641 |
| 著者（英） | Mahoney, W. A.; Ling, J. C.; Wheaton, W. A.; Jacobson, A. S. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 1985-08-01 |
| 言語 | eng |
| 内容記述 | A model based on 24 Mg(1369) was developed as the source of the lines in which refractory grains in the jets, containing Mg and 0, are bombarded, by ambient protons in the local ISM. The narrowness of the features results because the recoil Mg nucleus is stopped in the grain before the 1369 keV excited state decays. A consequence of the 24 Mg interpretation is the expected appearance of other emission lines, due to 20 Ne and 20 Na, which are produced by proton bombardment of 24 Mg at the 33 MeV/nucleon energy corresponding to the velocity of the jets. These lines appear at rest energies of 1634 keV and 1636 keV, respectively, and should have essentially the same total flux as that emited at 1369 keV. The HEAO 3 data are examined to search for the 1634 keV (rest) emission. The observation and analysis, the results, and the implications for the understanding of SS 433 are discussed. |
| NASA分類 | SPACE RADIATION |
| レポートNO | 85N33954
OG-2.4-9 |
| 権利 | No Copyright |
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