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

Sezer A., GÖK F., Hudaverdi M., Aktekin E., ERCAN E. N.

9th International Conference of the Hellenic-Astronomical-Society, Athens, Yunanistan, 20 - 24 Eylül 2009, cilt.424, ss.171-173 identifier

  • Yayın Türü: Bildiri / Tam Metin Bildiri
  • Cilt numarası: 424
  • Basıldığı Şehir: Athens
  • Basıldığı Ülke: Yunanistan
  • Sayfa Sayıları: ss.171-173
  • Orta Doğu Teknik Üniversitesi Adresli: Hayır

Özet

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.