Fig. 7
Top panels: the behavior of I(M) for rotating stars (from left to right f equals 0, 900, 1000, 1100 and 1200 Hz) for hyperonic EOSs and DH EOS for comparison. Bottom panels: allowable range of the moment of inertia for purely nucleonic stars (left) and hyperonic stars (right). Thin (thick) lines correspond to the minimum (maximum) of I that a stable configuration can attain at a given frequency. (Color online).
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