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Fig. 13.


Upper row, left panel: Comparison of tidal deformabilities Λ for stellar component masses compatible with the GW170817 observation (assuming low-spin priors; Abbott et al. 2017a). The shaded area denotes the estimated 90% confidence region corresponding to the measurement. Right panel: Stellar mass as a function of tidal deformability Λ, for the mass range between 1.15 M and the Mmax. Lower row, left panel: Tidal deformability Λ as a function of stellar radius; points denote 1.2, 1.4, and 1.6 M (from upper to lower). Approximate formula denoted in the text is represented by black dotted curves. Right panel: Mass as a function of the k2 tidal Love number.

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