タイトル | Observation of soft X-rays from extended sources |
本文(外部サイト) | http://hdl.handle.net/2060/19740027123 |
著者(英) | Catura, R. C.; Acton, L. W. |
著者所属(英) | Lockheed Missiles and Space Co. |
発行日 | 1974-06-30 |
言語 | eng |
内容記述 | Efforts were directed toward surveying several supernova remnants for the emission of soft X-rays. Rather than attempt to detect such faint X-ray emission, the program was redirected to observe the spectrum and angular structure of the extended X-ray source in the Perseus cluster of galaxies and the super-nova remnant Puppis A. An attempt was made to detect X-ray line emission from Puppis A with a Bragg crystal spectrometer. Observations provide evidence for the presence of X-ray line emission in the spectrum of Puppis A near .65 keV. |
NASA分類 | SPACE SCIENCES |
レポートNO | 74N35236 NASA-CR-140516 |
権利 | No Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/192516 |