Fig. 4.

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Left: difference of the adiabatic exponent, Γ1, from 4/3 as a function of Mr/M for selected models. Solid and dashed lines indicate unstable and stable models against the GR instability, respectively. Accretion rates are color-coded, as is indicated. Right: quantity, Q, defined in Eq. (12) is plotted as a function of Mr/M for the structures of SMSs with various accretion rates. Unstable and stable structures are plotted with solid and short-dashed lines, respectively. These curves are compared with the long-dashed black line representing Qcrit (Eq. (13)) that corresponds to the Q for the critical n = 3 polytrope.
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