Formation channels of gravitationally resolvable double white dwarf binaries inside globular clusters

Open Access

Fig. 1

Histograms of the binary property distributions. The blue bars represent the whole dataset (64 660 binaries), while the orange bars represent the resolvable binaries (3289 binaries). Panel a shows the semimajor axis, panel b shows the eccentricity, panels c and d show the primary and secondary mass, respectively, and panel e shows the mass ratio $(\frac{M 2}{M 1})$ $\left(\frac{M2}{M1}\right)$ .

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