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Table 2
Mass loss rates, Ṁ and angular momentum loss rates, 
, calculated from the steady-state solutions.
| Parameter | HD 1237 | HD 22049 | HD 147513 | Sun | |||
| ZDI | SH-ZDI | ZDI | SH-ZDI | SH-ZDI | CR 1922 (Min) | CR 1962 (Max) | |
|
|
|||||||
| Ṁ [× 10-14M⊙ yr-1] | 4.70 | 13.9 | 2.77 | 10.2 | 11.4 | 2.76 | 4.80 |
| [× 1030 erg] |
6.77 | 58.0 | 1.10 | 12.3 | 3.66 | 0.40 | 1.10 |
| ⟨ur⟩AS [km s-1] | 679 | 654 | 562 | 493 | 363 | 364 | 171 |
| ⟨n⟩AS [× 104 cm-3] | 2.85 | 3.09 | 2.65 | 3.64 | 15.1 | 4.97 | 30.0 |
| ⟨T⟩AS [× 106 K] | 2.33 | 1.52 | 1.81 | 1.34 | 1.54 | 1.26 | 0.84 |
| ⟨B⟩AS [× 10-2 G] | 1.94 | 2.08 | 1.82 | 2.23 | 2.98 | 1.64 | 2.63 |
| ⟨RAS⟩ [R∗] | 12.0 | 19.6 | 10.2 | 15.6 | 7.1 | 6.4 | 6.8 |
Notes. The additional stellar wind properties represent averages over the resulting Alfvén surface (AS), while ⟨RAS⟩ corresponds to the mean AS radius in each case.
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