The Abundance Inhomogeneity in the Northern Rim of the Cygnus Loop


We observed the northern rim of the Cygnus Loop with the Suzaku observatory in 5 pointings (P21-P25). From the spatially resolved analysis, all the spectra are well fitted by the single component of the non-equilibrium ionization plasma model. From the best-fit parameters, we found that the abundances of the heavy elements are significantly lower than the… (More)

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