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Table 7.
Properties of HerBS-89a derived from the dust continuum spectrum.
| Quantity | Value | Units |
|---|---|---|
| DL07 model | ||
| μLDL07(8 − 1000 μm) | (2.89 ± 0.25) 1013 | L⊙ |
| μMDL07 (dust) | (1.30 ± 0.07) 1010 | M⊙ |
| Optically thin MBB | ||
| TMBB,thin (dust) | 28.0 ± 1.3 | K |
| βMBB, thin | 2.01 ± 0.11 | – |
| μLMBB,thin(50 − 1000 μm) | (1.94 ± 0.08) 1013 | L⊙ |
| μMMBB,thin (dust) | (1.11 ± 0.06) 1010 | M⊙ |
| MBB in general form | ||
| TMBB,gen (dust) | 49.2 ± 2.7 | K |
| βMBB, gen | 2.24 ± 0.13 | – |
| ν0, MBB, gen | 1214 ± 121 | GHz |
| λ0, MBB, gen | 247 ± 24 | μm |
| μLMBB,gen(50 − 1000 μm) | (2.00 ± 0.08) 1013 | L⊙ |
| μMMBB,gen (dust) | (6.06 ± 0.71) 109 | M⊙ |
| De-magnified values from DL07 | ||
| LIR(8 − 1000 μm) | (4.6 ± 0.4) 1012 | L⊙ |
| Mdust | (2.6 ± 0.2) 109 | M⊙ |
Notes. The MBB results include the correction for the CMB effect on T and β. The last two rows are based on the DL07 model and have been corrected for the gravitational lens magnification.
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