Accretion from debris disks onto white dwarfs - Fingering (thermohaline) instability and derived accretion rates

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Table 1

Models of DA and DB white dwarfs.

Models	T_eff [K]	Log g	M_cz [g]	Type

1	10 600 K	7.90	1.68 × 10²¹	DAZ
2	12 800 K	7.88	1.82 × 10¹⁷	DAZ
3	16 900 K	7.80	^*3.52 × 10¹⁶	DAZ
4	10 600 K	8.02	1.84 × 10²⁸	DBZ
5	17 100 K	7.99	1.39 × 10²⁶	DBZ
6	21 110 K	7.98	2.70 × 10²⁴	DBZ

Notes.M_cz is the mass contained in the convective zone.

^(*)

This mass is arbitrarily defined because the model has no convective zone.

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