Gas- and dust evolution in protoplanetary disks | Astronomy & Astrophysics (A&A)

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Table 1:

Parameters of the fiducial model.
Parameter	Symbol	Value	Unit
turbulence parameter	$\alpha$	10^-3	-
irradiation angle	$\varphi$	0.05	-
cloud mass	$M_{\rm cloud}$	0.5	$M_\odot$
effect. speed of sound in core	$\ensuremath{c_{\rm s}}$	$3\ensuremath{\times 10^{4}}$	cm s^-1
rotation rate of cloud core	$\Omega_{\rm s}$	$7\ensuremath{\times 10^{-14}}$	s^-1
solid density of dust grains	$\rho _{\rm s}$	1.6	g cm^-3
stellar radius	$R_\star$	2.5	$R_\odot$
stellar temperature	$T_\star$	4000	K

Source LaTeX | All tables | In the text

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