Accretion rates of 42 nova-like stars with IUE and Gaia data

Open Access

Fig. 3.

Power-law index vs. the cosine of the inclination angle. The panels display the four correlations at p_H₀ < 10⁻², i.e., from the top the whole sample, the UX, VY, and SW classes, each with their respective correlation parameters and fits. The nSW class shows no correlation. V426 Oph is highlighted with a square box (see last paragraph of Sect. 6.2 for details).

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