Mass-radius relation of white dwarfs from close binary systems

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Table 2.

Selected models at T_eff = 50 kK.

Model	M_d [M_⊙]	R_d [10⁻² R_⊙]	P_orb [days]	M_H [10⁻⁴ M_⊙]
A	0.2967	6.8018	72.716	6.4218
C	0.3536	6.7347	271.192	8.2267

B	0.3010	6.0117	78.383	6.0070
E	0.2463	5.9779	6.424	2.1685

Notes. Details of the selected models at T_eff = 50 kK used for comparison in Figures 3, 4, and 6. Columns correspond to the label, donor mass, donor radius, orbital period of the system, and donor hydrogen mass.

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