Suzaku Analysis of Galactic Supernova Remnants G27.4+0.0 and G12.0-0.1

Sezer A., Gök F., Hüdaverdi M., Aktekin E., Ercan E. N.

wos, Athens, Greece, 20 - 24 September 2009, vol.424, pp.171-176, (Full Text)

  • Publication Type: Conference Paper / Full Text
  • Volume: 424
  • City: Athens
  • Country: Greece
  • Page Numbers: pp.171-176
  • Akdeniz University Affiliated: Yes

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 (N-H), electron temperature (kT(e)), ionization timescale (n(e)t) 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.