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We present the results of an X-ray spectral analysis of the northeast regionof the candidate supernova remnant G189.6+3.3 with Suzaku. K-shell lines fromhighly ionized Ne, Mg, Si, and S were detected in the spectrum for the firsttime. In addition, a radiative recombining continuum (RRC) from He-like Si wasclearly seen near 2.5 keV. This detection of an RRC reveals for the first timethat G189.6+3.3 possesses an X-ray-emitting recombining plasma (RP). Theextracted X-ray spectrum in the 0.6-10.0 keV energy band is well fitted with amodel consisting of a collisional ionization equilibrium plasma component(associated with the interstellar medium) and an RP component (associated withthe ejecta). The spectral feature shows that G189.6+3.3 is most likely to be amiddle-aged SNR with an RP.

Discovery of recombining plasma associated with the candidate supernova remnant G189.6+3.3 with Suzaku