Table 3
Brightest emission lines in the CND.
| Lines | Wavelengths (μm) | Model flux (W/m2/sr) | Measured flux (W/m2/sr) |
|---|---|---|---|
| 5.298–5.386 | 7.33 × 10–7 | 5.10 × 10–7 ± 5.00 × 10–9 | |
| Fe II | 5.339 | 7.33 × 10–7 | – |
| 5.474–5.562 | 1.31 × 10–6 | 6.85 × 10–7 ± 9.73 × 10–9 | |
| H2 | 5.510 | 1.22 × 10–6 | – |
| H2 | 5.554 | 8.60 × 10-8 | – |
| 6.091–6.180 | 4.74 × 10–7 | 2.33 × 10–7 ± 2.00 × 10–9 | |
| H2 | 6.107 | 4.67 × 10–7 | – |
| H2 | 6.101 | 6.68 × 10–9 | – |
| 6.621–6.709 | 4.28 × 10–7 | 1.36 × 10–7 ± 1.42 × 10–9 | |
| Ni II | 6.634 | 4.28 × 10–7 | – |
| 6.885–6.973 | 1.51 × 10–6 | 1.11 × 10–6 ± 9.20 × 10–9 | |
| Ni II | 6.918 | 1.51 × 10–6 | – |
| 6.973–7.062 | 1.00 × 10–5 | 6.53 × 10–6 ± 4.97 × 10–8 | |
| Ar II | 6.983 | 1.00 × 10–5 | – |
| 7.988–8.076 | 5.86 × 10–7 | 4.78 × 10–7 ± 2.89 × 10–9 | |
| H2 | 8.023 | 5.86 × 10–7 | – |
| 8.958–9.046 | 2.50 × 10–7 | 6.94 × 10–8 ± 4.84 × 10–10 | |
| Ar III | 8.989 | 2.50 × 10–7 | – |
| 12.265–12.354 | 2.71 × 10–7 | 2.23 × 10–7 ± 1.84 × 10–9 | |
| Fe VI | 12.307 | 2.10 × 10–7 | – |
| H2 | 12.275 | 6.06 × 10–8 | – |
| 12.795–12.883 | 1.58 × 10–5 | 1.60 × 10–5 ± 1.70 × 10–7 | |
| Ne II | 12.810 | 1.58 × 10–5 | – |
| 14.338–14.426 | 1.97 × 10–7 | 1.36 × 10–7 ± 1.41 × 10–9 | |
| Cl II | 14.364 | 1.97 × 10–7 | – |
| 15.529–15.617 | 6.77 × 10–7 | 6.46 × 10–7 ± 5.81 × 10–9 | |
| Ne III | 15.551 | 6.77 × 10–7 | – |
| 17.028–17.116 | 1.66 × 10–7 | 1.36 × 10–7 ± 1.12 × 10–9 | |
| H2 | 17.030 | 1.66 × 10–7 | – |
| 17.910–17.998 | 1.16 × 10–7 | 1.15 × 10–7 ± 1.08 × 10–9 | |
| Fe II | 17.931 | 1.16 × 10–7 | – |
| 18.704–18.792 | 2.29 × 10–6 | 2.79 × 10–6 ± 2.43 × 10–8 | |
| S III | 18.708 | 2.29 × 10–6 | – |
| 21.791–21.879 | 3.59 × 10–8 | 2.56 × 10–8 ± 1.69 × 10–10 | |
| Ar III | 21.825 | 3.59 × 10–8 | – |
| 22.893–22.981 | 6.21 × 10–7 | 8.98 × 10–7 ± 8.23 × 10–9 | |
| Fe III | 22.919 | 6.21 × 10–7 | – |
| 24.481–24.569 | 4.37 × 10–8 | 4.03 × 10–8 ± 4.40 × 10–10 | |
| Fe II | 24.513 | 4.37 × 10–8 | – |
| 25.231–25.319 | 5.01 × 10–8 | 4.39 × 10–8 ± 3.43 × 10–10 | |
| S I | 25.242 | 5.01 × 10–8 | – |
| 25.980–26.068 | 7.11 × 10–7 | 7.40 × 10–7 ± 9.39 × 10–9 | |
| Fe II | 25.981 | 7.11 × 10–7 | – |
Notes. List of the 20 brightest emission features detected in the CND spectrum, sorted by wavelength. For each feature, the wavelength interval, total flux from the model, and measured flux are listed in the top row. The subsequent rows indicate the individual emission lines predicted by the model within that interval, including their rest wavelengths and modeled fluxes. When several lines fall within the same spectral bin, they are all listed, illustrating the possible line blending. The modeled flux values are those from the best-fit multiphase model.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.