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Table 2
Modeled mass-loss rates Ṁ for different stellar XUV fluxes/spectra and lower boundary parameters (number density n0, temperature T0).
FXUV | XUV | n0 | T0 | Ṁ |
---|---|---|---|---|
(erg cm−2 s−1) | (cm−3) | (K) | (g s−1) | |
1.80 × 104 | SF11 | 1015 | 1200 | 5.4 × 1010 |
1.27 × 104 | L14 | 1015 | 1200 | 2.5 × 1010 |
3.65 × 104 | SF11+X | 1015 | 1200 | 8.7 × 1010 |
7.18 × 104 | SF11+XUV | 1015 | 1200 | 1.2 × 1011 |
1.80 × 104 | SF11 | 1015 | 800 | 4.8 × 1010 |
1.80 × 104 | SF11 | 1015 | 1600 | 6.1 × 1010 |
1.80 × 104 | SF11 | 5 × 1015 | 1200 | 1.7 × 1011 |
Notes. Rows 3 and 4 give the results for the X-ray and XUV flares, respectively (see Sect. 3.2).
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