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Spectra of G272.2-3.2 are well fitted by a single-temperature variable abundances non-equilibrium ionization (VNEI) model with an electron temperature kTe \\sim 0.77 keV, ionization timescale {\\tau} \\sim 6.5 \\times 10^10 cm-3 s and absorbing column density NH \\sim 1.1 \\times 10^22 cm-2. We have detected enhanced abundances of Si, S, Ca, Fe and Ni in the center region indicating that the X-ray emission has ejecta origin. 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Sezer, F. Gok","submitted_at":"2012-01-16T11:51:21Z","abstract_excerpt":"In this work, the results from Suzaku observation of Galactic supernova remnant G272.2-3.2 are presented. Spectra of G272.2-3.2 are well fitted by a single-temperature variable abundances non-equilibrium ionization (VNEI) model with an electron temperature kTe \\sim 0.77 keV, ionization timescale {\\tau} \\sim 6.5 \\times 10^10 cm-3 s and absorbing column density NH \\sim 1.1 \\times 10^22 cm-2. We have detected enhanced abundances of Si, S, Ca, Fe and Ni in the center region indicating that the X-ray emission has ejecta origin. 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