Table A.4.
Mass-loss rates, photodissociation radii, and wind densities of SRs in the sample for the optically thick and optically thin cases, respectively.
| Source | Spectral type | Ṁthick | Ṁthin |  |
 |
(Ṁ / Vexp)thick | (Ṁ / Vexp)thin |
|---|---|---|---|---|---|---|---|
| (M⊙ yr−1) | (M⊙ yr−1) | (1015 cm) | (1015 cm) | (M⊙ yr−1 km−1 s) | (M⊙ yr−1 km−1 s) | ||
| VX And | C | < 4.90−1.70 × 10−9 | < 1.94−0.68 × 10−9 | < 7.04−0.73 | < 5.61−0.48 | < 3.80−1.62 × 10−10 | < 1.50−0.64 × 10−10 |
| V370 And | M | 8.23 |
3.66 |
17.00 |
11.80 |
7.34 |
3.26 |
| Z Eri | M | < 1.89−0.71 × 10−9 | < 8.88−3.31 × 10−10 | < 3.85−0.43 | < 3.26−0.34 | < 2.43−1.23 × 10−10 | < 1.14−0.57 × 10−10 |
| SS Cep | M | 9.17 |
4.08 |
17.90 |
12.40 |
8.11 |
3.61 |
| TT Tau | C | 1.37 |
5.25 |
27.00 |
16.60 |
1.61 |
6.20 |
| W Ori | C | 5.91 |
2.27 |
57.30 |
34.60 |
4.92 |
1.89 |
| RX Lep | M | 3.06 |
1.44 |
10.20 |
7.20 |
5.41 |
2.54 |
| Y Tau | C | 5.79 |
2.22 |
55.50 |
34.10 |
3.42 |
1.31 |
| S Lep | M | < 2.11−0.73 × 10−9 | < 9.89−3.47 × 10−10 | < 4.58−0.42 | < 3.97−0.34 | < 2.04−0.90 × 10−10 | < 9.58−4.28 × 10−11 |
| RY Mon | C | 3.65 |
1.40 |
44.30 |
27.10 |
2.97 |
1.14 |
| RT Hya | M | 2.52 |
1.32 |
3.26 |
2.58 |
6.63 |
3.46 |
| RT Cnc | M | < 9.39−3.35 × 10−10 | < 4.34−1.50 × 10−10 | < 3.53−0.34 | < 3.13−0.29 | < 1.08−0.51 × 10−10 | < 4.97−2.29 × 10−11 |
| R Crt | M | 2.28 |
1.01 |
27.90 |
18.80 |
1.91 |
8.50 |
| Z UMa | M | < 9.20−4.05 × 10−10 | < 4.89−2.03 × 10−10 | < 2.25−0.38 | < 1.87−0.31 | < 2.54−1.82 × 10−10 | < 1.35−0.93 × 10−10 |
| BK Vir | M | 2.39 |
1.12 |
9.17 |
6.56 |
3.81 |
1.79 |
| Y UMa | M | 9.53 |
4.24 |
18.00 |
12.10 |
1.35 |
6.00 |
| Y CVn | C | 5.00 |
1.92 |
16.30 |
10.60 |
5.10 |
1.96 |
| RT Vir | M | 4.85 |
2.15 |
41.40 |
27.10 |
4.69 |
2.09 |
| SW Vir | M | 3.62 |
1.61 |
35.70 |
23.40 |
3.84 |
1.71 |
| RX Boo | M | 6.49 |
2.89 |
15.20 |
10.70 |
5.84 |
2.60 |
| τ4 Ser | M | 5.96 |
2.65 |
15.70 |
11.70 |
3.41 |
1.52 |
| ST Her | M | 1.09 |
4.87 |
19.50 |
13.60 |
8.79 |
3.91 |
| X Her | M | 6.81 |
3.03 |
15.40 |
10.70 |
6.71 |
2.98 |
| G Her | M | 1.50 |
6.91 |
8.69 |
6.85 |
1.17 |
5.40 |
| S Dra | M | 1.26 |
5.60 |
20.80 |
14.20 |
1.17 |
5.20 |
| FI Lyr | M | 1.38 |
6.15 |
21.70 |
14.60 |
1.60 |
7.11 |
| S Sct | C | 2.23 |
9.02 |
11.00 |
7.41 |
2.95 |
1.19 |
| AF Cyg | M | 1.36 |
6.29 |
7.06 |
5.13 |
2.30 |
1.06 |
| AQ Sgr | C | 1.90 |
7.28 |
31.60 |
19.70 |
1.60 |
6.15 |
| RT Cap | C | 4.14 |
1.60 |
14.80 |
9.67 |
4.60 |
1.78 |
| UU Dra | M | 1.90 |
8.46 |
25.50 |
17.20 |
1.65 |
7.32 |
| EU Del | M | 5.80 |
2.64 |
6.34 |
5.25 |
4.83 |
2.20 |
| U Del | M | 7.54 |
3.35 |
16.30 |
11.40 |
6.77 |
3.01 |
| IQ Aqr | M | 1.15 |
5.28 |
7.97 |
6.38 |
8.97 |
4.12 |
| W Cyg | M | 4.20 |
1.91 |
12.30 |
8.78 |
4.44 |
2.02 |
| RU Cyg | M | 2.79 |
1.24 |
30.80 |
20.70 |
2.24 |
9.95 |
| EP Aqr | M | 1.19 |
5.31 |
20.30 |
14.00 |
9.80 |
4.36 |
| TW Peg | M | 9.44 |
4.20 |
18.20 |
12.70 |
7.64 |
3.39 |
| SV Lyn | M | 4.76 |
2.35 |
4.10 |
3.01 |
1.63 |
8.05 |
| SV Peg | M | 1.07 |
4.75 |
64.10 |
41.30 |
1.18 |
5.24 |
| AK Hya | M | 1.68 |
7.82 |
7.96 |
5.85 |
2.32 |
1.08 |
| RW Boo | M | 9.89 |
4.40 |
19.30 |
13.90 |
5.72 |
2.54 |
| IQ Her | M | 1.66 |
7.73 |
7.84 |
5.72 |
2.48 |
1.15 |
| AA Cyg | S | 1.56 |
6.25 |
27.50 |
17.00 |
2.55 |
1.02 |
| X Cnc | C | 2.87 |
1.10 |
40.00 |
24.10 |
3.49 |
1.34 |
| V465 Cas | M | 4.69 |
2.11 |
13.10 |
9.38 |
4.38 |
1.97 |
Notes. Description of the columns from left to right: (1–2) GCVS designation and spectral type (Samus et al. 2009); (3–8) Mass-loss rate, photodissociation radius, and surface wind density estimates with the corresponding asymmetric uncertainties for the optically thick and optically thin case, respectively. 3σ upper detection limits are indicated.
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