Table 2
Mass (ejecta plus disk) gravitationally bound to the secondary star, ΔMMS, and to the white dwarf, ΔMWD, and total mass leaving the binary system, ΔMesc, together with their fractions (in %) over the total ejecta plus disk masses, after collision with the nova ejecta. The parameter Δ MMS,lost is the mass lost by the main sequence star in the interaction with the nova ejecta.
| Model | Δ MMS (M⊙) | Δ MWD (M⊙) | Δ Mesc (M⊙) |  |
 |
 |
ΔMMS, lost(M⊙) |
|---|---|---|---|---|---|---|---|
| A | 1.95 × 10−5 | 4.64 × 10−5 | 4.69 × 10−4 | 3.65% | 8.68% | 87.7% | 2 × 10−7 |
| Ahres | 2.05 × 10−5 | 4.83 × 10−5 | 4.66 × 10−4 | 3.83% | 9.03% | 87.2% | 1.4 × 10−7 |
| B | 2.92 × 10−5 | 1.01 × 10−4 | 4.05 × 10−4 | 5.46% | 18.9% | 75.6% | – |
| C | 4.96 × 10−5 | 1.50 × 10−4 | 4.08 × 10−4 | 8.17% | 24.7% | 67.2% | 1.6 × 10−7 |
| D | 6.20 × 10−5 | 1.83 × 10−4 | 3.62 × 10−4 | 10.2% | 30.2% | 59.7% | 1.2 × 10−7 |
| E | 5.62 × 10−5 | 1.12 × 10−4 | 1.45 × 10−3 | 3.47% | 6.93% | 89.7% | 1.4 × 10−6 |
| F | 9.82 × 10−5 | 2.66 × 10−4 | 1.26 × 10−3 | 6.06% | 16.4% | 77.6% | 4.8 × 10−7 |
| G | 5.69 × 10−5 | 1.71 × 10−4 | 3.26 × 10−4 | 10.3% | 30.9% | 58.9% | 4 × 10−8 |
| H | 6.06 × 10−5 | 1.25 × 10−4 | 1.46 × 10−3 | 3.69% | 7.60% | 88.8% | 1.3 × 10−6 |
| I | 2.17 × 10−5 | 4.79 × 10−5 | 5.40 × 10−4 | 3.57% | 7.88% | 88.9% | 2.4 × 10−6 |
| J | 1.66 × 10−5 | 5.55 × 10−5 | 4.83 × 10−4 | 3.00% | 10.0% | 87.2% | 1.4 × 10−6 |
| K | 5.39 × 10−5 | 1.61 × 10−4 | 3.20 × 10−4 | 10.1% | 30.1% | 59.8% | – |
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.