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

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

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..424..171s&link_type=abstract

Proceedings of the 9th International Conference of the Hellenic Astronomical Society, proceedings of a conference held 20-24 Sep

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Suzaku Analysis of Galactic Supernova Remnants G27.4+0.0 and G12.0-0.1 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Suzaku Analysis of Galactic Supernova Remnants G27.4+0.0 and G12.0-0.1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Suzaku Analysis of Galactic Supernova Remnants G27.4+0.0 and G12.0-0.1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-953913