Rate of WD-WD head-on collisions in isolated triples is too low to explain standard type Ia supernovae

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Table 1

Distributions of the initial binary masses and orbital parameters for the different models.

Model	q_inner	q_outer	a_inner	a_outer	e_inner	e_outer
STD	uniform	uncorrelated	log-uniform¹	log-uniform	thermal²	thermal
Q_IN	uncorrelated	uncorrelated	log-uniform	log-uniform	thermal	thermal
Q_OUT	uniform	uniform	log-uniform	log-uniform	thermal	thermal
A_SANA	uniform	uncorrelated	power-law³	power-law	thermal	thermal
A_RIZ	uniform	uncorrelated	log-normal⁴	log-normal	thermal	thermal
E_CIRC	uniform	uncorrelated	log-uniform	log-uniform	0	0

References. ⁽¹⁾ Abt (1983); ⁽²⁾ Heggie (1975); ⁽³⁾ Sana et al. (2012); ⁽⁴⁾ Rizzuto et al. (2013).

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