| タイトル | SWS and LWS observations of Cassiopeia A |
| 著者（英） | Unger, S. J.; Lahuis, F.; Cox, P.; Haas, M. R.; Baluteau, J. P.; Pequignot, D.; Emery, R. J.; Morisset, C. |
| 著者所属（英） | NASA Ames Research Center |
| 発行日 | 1997-12-01 |
| 言語 | eng |
| 内容記述 | The observations of the Casssiopeia A supernova remnant performed with the short wavelength spectrometer (SWS) and the long wavelength spectrometer (LWS), onboard the Infrared Space Observatory (ISO), are reported on. Broad O III 52 micrometer and 88 micrometer and O I 63 micrometer emission lines were detected. The far infrared O III lines fit the model of a spherical shell with central velocity redshifted by 770 +/- 40 km/s. A pronounced density contrast between the front and back of the shell was detected. |
| NASA分類 | Astrophysics |
| 権利 | No Copyright, Distribution within the U.S. granted by agreement |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/540831 |
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