Bondi accretion for adiabatic flows onto a massive black hole with an accretion disc - The one dimensional problem

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201935917e]

Table 1.

Parameters of the generalized Bondi accretion models.

Run	Lines ^(a)	f_⋆	f_disc	γ	θ^phase			x_crit
					(rad)	(rad)	(rad)
	Yes	0.50	0.50	1.1	0.517465	1.1	0.9	0.00856
	Yes	0.20	0.80	1.1	0.821151	1.1	0.9	0.03350
	Yes	0.05	0.95	1.1	0.886684	1.1	0.9	0.04559
M₁	No	0.50	0.50	1.1	NA	1.1	0.9	0.12149
M₂	No	0.20	0.80	1.1	0.391333	1.1	0.9	0.00571
M₃	No	0.05	0.95	1.1	0.540618	1.1	0.9	0.01332

Notes.

^(a)

M(τ)≠0 (yes) and M(τ) = 0 (no). The angles and are given in terms of θ^phase, i.e., and .

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