Cool circumgalactic gas of passive galaxies from cosmological inflow

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Table 3.

MCMC results of the two additional models.

Model	log (m_cl, start/M_⊙)	α	f_accr
		(Gyr⁻¹)
r_destr = r_vir/2
r_start = r_vir/2

Notes. 50th percentiles (with errors given by the 32nd and the 68th percentiles) of the posterior distributions of the three parameters obtained with the MCMC fits performed for models with r_destr = r_vir/2 (Sect. 6.1) and r_start = r_vir/2 (Sect. 6.3).

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