| タイトル | Observations of x ray pulsars from the Kvant module |
| 著者（英） | Melioranskiy, A.; Churazov, E.; Sunyaev, Rashid A.; Yamburenko, N.; Efremov, V. V.; Loznikov, V.; Kaniovskiy, A.; Gilfanov, M.; Skinner, G. K.; Kuznetsov, A. V. |
| 著者所属（英） | Tuebingen Univ.|Academy of Sciences (USSR)|Birmingham Univ.|Max-Planck-Inst. fuer Physik und Astrophysik|Space Research Organization Netherlands |
| 発行日 | 1991-01-01 |
| 言語 | eng |
| 内容記述 | The Roentgen international x ray observatory on the Kvant module of the Mir space station has been successfully operating since the beginning of June 1987. Many x ray sources were observed and among them were several x ray pulsars. Four telescopes mounted on board the Kvant module cover a wide energy range with good timing resolution. Timing analysis of the Kvant module data suffers from the presence of only short continuous intervals of source observations, separated by 90 min gaps (90 min is the orbital period of the Mir space station around the Earth). The presence of 90 min gaps leads to the appearance of beat frequencies v=v sub 0 + or - n/90 min (n = 1, 2, 3). Special analysis was applied to avoid this difficulty. Results are presented of the pulsation period measurements of the x ray pulsars Her X-1, Cen X-3, SMC X-1, Vela X-1, A0535 + 26 by the instruments on board the Kvant module in 1987 to 1989. The values of the periods are reduced to the solar system barycenter and to the binary system barycenter (excluding A0535 + 26). |
| NASA分類 | SPACE RADIATION |
| レポートNO | 92N12949 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/525181 |
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