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Table 7:

Parameters involved in the TLTD model.

Parameter
Meaning

$F_\nu$
Observed flux
$F_{\rm\nu, cont}$ Total continuum flux
d Distance to the source
R* Stellar radius
T* Stellar temperature
D0 Contribution of the star to the total flux
D1 Contribution of the inner rim to the total flux
D2 Contribution of the midplane to the total flux
Di,j Mass contribution of species i with size j
$T_{a,\ \rm out}$ Lowest temperature in the disk atmosphere
$T_{a,\ \rm in}$ Highest temperature in the disk atmosphere
$T_{r,\ \rm out}$ Lowest temperature in the inner rim
$T_{r,\ \rm in}$ Highest temperature in the inner rim
$T_{m,\ \rm out}$ Lowest temperature in the disk midplane
$T_{m,\ \rm in}$ Highest temperature in the disk midplane
$\kappa_{i,j}$ Mass absorption coefficient of species i with size j
qr Power exponent of the temperature distribution (as a function of radius) in the rim
qa Power exponent of the temperature distribution (as a function of radius) in the disk atmosphere
qm Power exponent of the temperature distribution (as a function of radius) in the disk midplane

Source LaTeX | All tables | In the text

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