X-ray observations of Vela-X |
| |
| Authors: | A Smith HU Zimmermann |
| |
| Institution: | 1. Astrophysics Division, Space Science Department of the European Space Agency, ESTEC, 2200AG Noordwijk, The Netherlands;2. Max-Plank-Institut für extraterrestrische Physik, 8046 Garching, F.R.G. |
| |
| Abstract: | Exosat ME observations of the Vela-X region are presented. It is found that the 2–10 keV emission is divided into two components. One is associated with the rulsar but is probably extended by 10–20 arc minutes, the other is associated with the Vela-X radio nebula and is probably more extended (). The Vela-X component is softer than the pulsar component. No pulsed emission is observed. |
| |
| Keywords: | |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
