TUBİTAK Adresli Yayınlar Topluluğu
Published January 1, 2010 | Version v1
Conference paper Open

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

Creators

  • 1. Akdeniz Univ, Dept Phys, TR-07058 Antalya, Turkey
  • 2. Space Technol Res Inst, TUBITAK, METU Campus, TR-06531 Ankara, Turkey
  • 3. Bogazici Univ, Dept Phys, TR-34342 Istanbul, Turkey

Description

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.

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