Vertical dissipation profiles and the photosphere location in thin and slim accretion disks

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Table 1:

Model assumptions for $\dot m=0.1~\dot m_{\rm C}$ .
Model	Model family^a	$\alpha$	$d_{\rm max}$	$d_{\rm disp}$	a^*
A1	$\alpha P$	0.001	-	-	0.0
A2	$\alpha P$	0.01	-	-	0.0
A3	$\alpha P$	0.1	-	-	0.0
A4	$\alpha P$	0.2	-	-	0.0
A5	$\alpha P$	0.5	-	-	0.0
A6	$\alpha P$	1.0	-	-	0.0
AS1	$\alpha P$	0.01	-	-	0.9
AS2	$\alpha P$	0.1	-	-	0.9
AS3	$\alpha P$	0.5	-	-	0.9
B1	constant diss. rate	0.01^b	-	-	0.0
B2	constant diss. rate	0.1^b	-	-	0.0
B3	constant diss. rate	0.5^b	-	-	0.0
C1	m^-1/2	0.01^b	-	-	0.0
C2	m^-1/2	0.1^b	-	-	0.0
C3	m^-1/2	0.5^b	-	-	0.0
D1	arbitrarily positioned	0.1	0.0	0.001	0.0
D2	arbitrarily positioned	0.1	0.02	0.001	0.0
D3	arbitrarily positioned	1.0	0.0	0.001	0.0
D4	arbitrarily positioned	1.0	0.02	0.001	0.0
D5	arbitrarily positioned	1.0	0.02	0.0005	0.0
D6	arbitrarily positioned	1.0	0.02	0.005	0.0

^a Details of model assumptions are given in Sect. 5.1; ^b calculated based
on surface density profiles obtained in the $\alpha P$ model with given $\alpha$ and a^*.

Source LaTeX | All tables | In the text

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