Suzaku Observations of Young Supernova Remnants

Details Suzaku Observations of Young Supernova Remnants Suzaku Observations of Young Supernova Remnants

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..137t&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Astronomy and Astrophysics

Astronomy

1

Supernova Remnants, Nucleosynthesis, X-Ray Sources (Astronomical), Satellites, Artificial, Supernova Remnants, Origin, Formation, And Abundances Of The Elements, X-Ray Sources, X-Ray Bursts, Artificial Earth Satellites

Scientific paper

We have observed several young supernova remnants with the Japanese X-ray satellite Suzaku to study the nucleosynthesis in supernova explosions. We have discovered very low abundant elements, chromium, manganeese, for the first time in Tycho's Kepler's and N103B supernova remants. We also found nickel in Kepler's supernova remant. The production yield of those metals tells us the nucleosynthesis in the thermonuclear explosive supernovae metallicity environment at the progenitor stars were born.

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