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We report the Suzaku/XIS results of the Galactic oxygen-rich supernovaremnant (SNR), G292.0+1.8, a remnant of a core-collapse supernova. The X-rayspectrum of G292.0+1.8 consists of two type plasmas, one is in collisionalionization equilibrium (CIE) and the other is in non-equilibrium ionization(NEI). The CIE plasma has nearly solar abundances, and hence would beoriginated from the circumstellar and interstellar mediums. The NEI plasma hassuper-solar abundances, and the abundance pattern indicates that the plasmaoriginates from the supernova ejecta with a main sequence of 30-35 Msolar. IronK-shell line at energy of 6.6 keV is detected for the first time in the NEIplasma.

Suzaku Discovery of Fe K-Shell Line from the O-Rich SNR G292.0+1.8