Table 1.
Resulting parameters of modeling the 
values via function (5).
| i | E/I(a) | n1 | nK | K |
 |
Ṁsp(b) |  (c) |
Object | d | Ṁ | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 70° | E |
 |
 |
 |
 |
 |
0.47 | BF Cyg | 3.4 | < 3.3 × 10−7(d) | (1) |
| I |
 |
 |
 |
 |
CI Cyg | 1.6 | ∼4.4 × 10−7 | (2) | |||
| 80° | E |
 |
 |
 |
 |
 |
0.35 | YY Her | 6.3 | < 2.9 × 10−7 | (3) |
| I |
 |
 |
 |
 |
AR Pav | 4.9 | – | (4) | |||
| 90° | E |
 |
 |
 |
 |
 |
0.43 | AX Per | 1.7 | ∼8.8 × 10−8 | (5) |
| I |
 |
 |
 |
 |
PU Vul | 4.7 | < 5.8 × 10−7(d) | (6) |
Notes. The first part of the table contains the fitting parameters of the wind, n1(1023 cm−2), nK(1025 cm−2), K, 
cm−2), the corresponding spherical equivalent of the mass-loss rate, Ṁsp (M⊙ yr−1; see Sect. 3.1), and a minimum of the 
function for three different orbital inclinations, i (see Sect. 2.2). The second part, to the right of the vertical bar, compares the total mass-loss rates, Ṁ (M⊙ yr−1), derived from radio emission by Seaquist et al. (1993) recalculated for distances d (in kpc) from the literature, listed in the last column, reference.
From egress (E) or ingress (I) data (see Sect. 2.2).
References. (1) Muerset et al. (1991), (2) Seaquist et al. (1993), (3) Skopal (2005a), (4) Schild et al. (2001), (5) Skopal et al. (2001), and (6) Kato et al. (2012).
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