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