XMM-Newton observation of the Vela pulsar
Abstract
We present the results from 90 ksec observation of the Vela pulsar with XMM-Newton. We put emphasis on studying emission from the pulsar. Based on highly-sensitive data, we conducted the following analysis: (1) high resolution spectroscopy by RGS in search for atmospheric spectral features (2) phase-resolved spectral analysis and energy-resolved timing analysis by EPIC-PN. We will discuss implications from the results.
- Publication:
-
34th COSPAR Scientific Assembly
- Pub Date:
- 2002
- Bibcode:
- 2002cosp...34E2643M