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Table 3

Radiative transfer models of IRS 9A.

Parameters Best SED-only fita Vehoff+2010 Best V2 model
(No. 3006825)b (No. 3012790)b (this work)

Total luminosity (L) 1.0 × 105 9.2 × 104 8.0 × 104
Stellar mass (M) 27.2 25.4 30.0
Stellar temperature (K) 39 000 38 500 38 000
Disk massc (M) 1.8 × 10-1 5.0 × 10-1 5.0 × 10-1
Disk outer radius (AU) 91.0 94.0 80.0
Disk inner radius (AU) 28.0 25.0 10.0
Disk flaring power –β 1.1 1.2 1.2
Disk scale height at 100 AU –h 8.9 8.8 8.0
Envelope outer radius (AU) 1.0 × 105 1.0 × 105 7 × 103
Envelope cavity angle (deg)d 31.0 29.0 30.0
Bipolar cavity density (g/cm3) 7.7 × 10-21 9.9 × 10-21 1.0 × 10-20
Inclination –i– (deg)e 87.0 85.0 60.0
Position Angle –φ– (deg)f 105.0g 105.0 120.0

Notes.

(a)

This is the best-fit model to the SED obtained with Robitaille’s online fitting tool.

(b)

Number of the model from Robitaille’s database.

(c)

Total mass (dust+gas).

(d)

Half-opening angle of a conical cavity in the envelope.

(e)

Inclination angle of the disk-envelope from the line of sight: 0° means that the disk and envelope are seeing face-on, 90° means that the disk and envelope are seeing edge-on.

(f)

Position angle of the disk mid-plane projected in the plane of the sky, measured East of North.

(g)

Assumed to be the same as Vehoff et al. (2010).

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