MBM 12: young protoplanetary discs at high galactic latitude

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Volume 497 / No 2 (April II 2009)

A&A, 497 2 (2009) 379-392

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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
D_i,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

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