Long-period thermal oscillations in superfluid millisecond pulsars

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Fig. 2

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Real and imaginary parts of the growth rates γ₊ and γ₋ (upper panel) calculated from Eq. (26) and components of the Jacobian matrix (lower panel) in Eqs. (22)–(25), for different values of Δ_n. In both panels, the stellar parameters are the same as in Fig. 1 and we assume that .

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