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Table 2.
Main results of this work for 46 SRs of the sample.
| Source | Spectral | Ṁ | RCO | Comments |
|---|---|---|---|---|
| type | (M⊙ yr−1) | (1015 cm) | ||
| VX And | C | < 1.94−0.68 × 10−9 | < 5.61−0.48 | Optically thin emission. Overly low mass-loss rate. |
| V370 And | M | 3.66 |
11.80 |
Optically thin emission. SHAPE+shapemol model (see below). |
| Z Eri | M | < 8.88−3.31 × 10−10 | < 3.26−0.34 | Optically thin emission. Overly low mass-loss rate. |
| SS Cep | M | 4.08 |
12.40 |
Optically thin emission. Low mass-loss rate. |
| TT Tau | C | 5.25 |
16.60 |
Optically thin emission. Low mass-loss rate. |
| W Ori | C | 5.91 |
57.30 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| RX Lep | M | 1.44 |
7.20 |
Optically thin emission. Low mass-loss rate. |
| Y Tau | C | 5.79 |
55.50 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| S Lep | M | < 9.89−3.47 × 10−10 | < 3.97−0.34 | Optically thin emission. Overly low mass-loss rate. |
| RY Mon | C | 3.65 |
44.30 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| RT Hya | M | 1.32 |
2.58 |
Optically thin emission. Overly low mass-loss rate. |
| RT Cnc | M | < 4.34−1.50 × 10−10 | < 3.13−0.29 | Optically thin emission. Overly low mass-loss rate. |
| R Crt | M | 2.28 |
27.90 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| Z UMa | M | < 4.89−2.03 × 10−10 | < 1.87−0.31 | Optically thin emission. Overly low mass-loss rate. |
| BK Vir | M | 1.12 |
6.56 |
Optically thin emission. SHAPE+shapemol model (see below). |
| Y UMa | M | 4.24 |
12.10 |
Optically thin emission. Low mass-loss rate. |
| Y CVn | C | 1.92 |
10.60 |
Optically thin emission. Low mass-loss rate. |
| RT Vir | M | 4.85 |
41.40 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| SW Vir | M | 3.62 |
35.70 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| RX Boo | M | 6.49 |
15.20 |
Optically thick emission. SHAPE+shapemol model (see below). |
| τ4 Ser | M | 2.65 |
11.70 |
Optically thin emission. SHAPE+shapemol model (see below). |
| ST Her | M | 1.09 |
19.50 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| X Her | M | 3.03 |
10.70 |
Optically thin emission. Similar to the case of V370 And (see below). |
| g Her | M | 6.91 |
6.85 |
Optically thin emission. Overly low mass-loss rate. |
| S Dra | M | 1.26 |
20.80 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| FI Lyr | M | 6.15 |
14.60 |
Optically thin emission. Similar to the case of BK Vir (see below). |
| S Sct | C | 9.02 |
7.41 |
Optically thin emission. Overly low mass-loss rate. |
| AF Cyg | M | 6.29 |
5.13 |
Optically thin emission. Overly low mass-loss rate. |
| AQ Sgr | C | 7.28 |
19.70 |
Optically thin emission. SHAPE+shapemol model (see below). |
| RT Cap | C | 1.60 |
9.67 |
Optically thin emission. Low mass-loss rate. |
| UU Dra | M | 1.90 |
25.50 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| EU Del | M | 2.64 |
5.25 |
Optically thin emission. Overly low mass-loss rate. |
| U Del | M | 3.35 |
11.40 |
Optically thin emission. Low mass-loss rate. |
| IQ Aqr | M | 5.28 |
6.38 |
Optically thin emission. Overly low mass-loss rate. |
| W Cyg | M | 1.91 |
8.78 |
Optically thin emission. Low mass-loss rate. |
| RU Cyg | M | 2.79 |
30.80 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| EP Aqr | M | 5.31 |
14.00 |
Optically thin emission. Similar to the case of V370 And (see below). |
| TW Peg | M | 4.20 |
12.70 |
Optically thin emission. Low mass-loss rate. |
| SV Lyn | M | 2.35 |
3.01 |
Optically thin emission. Overly low mass-loss rate. |
| SV Peg | M | 1.07 |
64.10 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| AK Hya | M | 7.82 |
5.85 |
Optically thin emission. Overly low mass-loss rate. |
| RW Boo | M | 4.40 |
13.90 |
Optically thin emission. Low mass-loss rate. |
| IQ Her | M | 7.73 |
5.72 |
Optically thin emission. Overly low mass-loss rate. |
| AA Cyg | S | 6.25 |
17.00 |
Optically thin emission. Low mass-loss rate. |
| X Cnc | C | 2.87 |
40.00 |
Optically thick emission. Similar to the case of RX Boo (see below). |
| V465 Cas | M | 2.11 |
9.38 |
Optically thin emission. Low mass-loss rate. |
Notes. Description of the columns from left to right. (1) GCVS designation (Samus et al. 2009); (2) spectral type from the GCVS (Samus et al. 2009); (3–4) conclusive mass-loss rate estimate and final photodissociation radius for each source in conformity with a simple test using SHAPE+shapemol (see below); (5) comments.
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