Radiation thermo-chemical models of protoplanetary disks - II. Line diagnostics

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Table 6:

Observed fluxes for MWC480.
Type	$\lambda$	Flux	Reference
O I	63 $\mu$ m	$\leqslant$ $1.1\times 10^{-15}$ W/m²/ $\mu$ m	1
O I	145 $\mu$ m	$\leqslant$ $1.8\times 10^{-16}$ W/m²/ $\mu$ m	1
C II	158 $\mu$ m	$5.9\pm 0.6\times 10^{-16}$ W/m²	1
		$5.5\pm 0.4\times 10^{-16}$ W/m²	2
CO	345 GHz	2.88 K km s^-1	3
		$4.23\times 10^{-19}$ W/m²	*
cont.	1.3 mm	$360\pm24$ mJy	4
cont.	2.7 mm	$39.9\pm 0.8$ mJy	4

References. (1) Creech-Eakman et al. (2002); (2) Lorenzetti et al. (2002); (3) Thi et al. (2004); (4) Mannings & Sargent (1997). (*) $\int T_{\rm mb}~{\rm d}v = 10^{-2} ~ \lambda_{\rm cm}/(2k) ~ (\Omega_a)^{-1} \int F_\nu({\rm W/m^2/Hz})~{\rm d}\nu$ , with $\Omega_a$ being the solid angle of the beam, i.e. $\pi (13.7''/2)^2$ for the JCMT.

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