Suzaku Analysis of Galactic Supernova Remnants G27.4+0.0 and G12.0-0.1
Abstract
We present Suzaku results of galactic supernova remnants (SNRs) G27.4 +0.0 and G12.0-0.1. From the spectra some important parameters like galactic hydrogen column density (NH), electron temperature (kTe), ionization timescale (net) are calculated. Furthermore, the abundances of Mg, Si, S are derived from the spectra of G27.4+0.0 indicating that G27.4+0.0 has originated from a core-collapse supernova explosion.
- Publication:
-
9th International Conference of the Hellenic Astronomical Society
- Pub Date:
- July 2010
- Bibcode:
- 2010ASPC..424..171S