Table 4
Properties of the adiabatically expanding synchrotron source components.
| Quantity | Sm | α | θ | νm | SNIR,SYN | SNIR,SSC | SX - ray | B | t0 | vexp | ||
|
|
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| Units | Jy | RS | GHz | mJy | mJy | nJy | G | UT h | c | |||
|
|
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| Uncertainty | 20% | 0.2 | 0.15 | 20% | 10% | 10% | 10% | 20% | 0.1 | 0.0015 | ||
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| A | 0.85 | +0.92 | 0.76 | 700 | 6.7 | 0.13 | 37 | 48 | 9.78 | 0.010 | ||
| B | 2.80 | +1.11 | 1.10 | 900 | 10.6 | 1.19 | 63 | 75 | 10.58 | 0.010 | ||
| C | 0.2 | +0.84 | 1.18 | 125 | 0.56 | <0.01 | <2 | 5 | 10.58 | 0.010 | ||
Notes. Listed are: peak flux Sm, spectral index α, sources size θ, peak frequency νm, NIR synchrotron flux SNIR,SYN, NIR SSC flux SNIR,SSC, X-ray flux SX - ray, magnetic field B, time of birth (UT hours), and expansion velocity vexp. The flux density uncertainty in the C component could be higher, and is mainly constrained by the CARMA data.
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