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Table 1
Sources by spectral type in ascending MLR order.
| Source | Variability type | Ṁ [M⊙ yr−1] | υ∞ [km s−1] | D [pc] |  [pc] |
|---|---|---|---|---|---|
| S-type semi-regulars and irregular stars(1): | |||||
| T Cet | SRc | 4 × 10−8 | 5.5 | 240 | 252 |
| Z Ant | SRb | 9 × 10−8 | 6.0 | 470 | 936 |
| UY Cen | SRb | 1.30 × 10−7 | 12.0 | 590 | 664 |
| AM Cen | SRb | 1.50 × 10−7 | 3.2 | 750 | 907 |
| ST Sco | SRa | 1.50 × 10−7 | 5.5 | 380 | 623 |
| FU Mon | SR | 2.70 × 10−7 | 2.8 | 780 | 789 |
| NSV 24 833 | U | 3 × 10−7 | 8.7 | 610 | 1106 |
| DY Gem | SRa | 7 × 10−7 | 8.0 | 680 | 906 |
| RZ Sgr | SRb | 3 × 10−6 | 9.0 | 730 | 424 |
| S-type Mira stars(1): | |||||
| TT Cen | M | 2.50 × 10−6 | 20.0 | 880 | 1348 |
| GI Lup | M | 5.50 × 10−7 | 10.0 | 690 | 1085 |
| RT Sco | M | 4.50 × 10−7 | 11.0 | 270 | 756 |
| IRC-10 401 | M | 3.50 × 10−7 | 17.0 | 430 | 2062 |
| ST Sgr | M | 2 × 10−7 | 6.0 | 540 | 542 |
| T Sgr | M | 1.40 × 10−7 | 7.5 | 590 | 3922 |
| W Aql | M | 2.20 × 10−6 | 17.2 | 230 | 375 |
| M-type semi-regulars and irregular stars(2,3,4): | |||||
| θ Aps | SRb | 4 × 10−8 | 4.5 | 110 | 119 |
| R Dor(*) | SRb | 1.30 × 10−7 | 5.5 | 45 | – |
| U Men | SRa | 2 × 10−7 | 7.2 | 320 | 325 |
| M-type Mira stars(2, 3, 4): | |||||
| IRC-30 398(*) | M: | 1.10 × 10−5 | 16.0 | 600 | 926 |
| C-type semi-regular and irregular stars(2,3,4): | |||||
| V1302 Cen | SRb | 1 × 10−7 | 6.5 | 530 | 911 |
| V996 Cen | SR | 1 × 10−7 | 11.0 | 390 | 576 |
| X TrA | Lb | 1.30 × 10−7 | 6.5 | 360 | 350 |
| AQ Sgr | SRb | 2.50 × 10−7 | 10.0 | 200 | – |
| C-type Mira stars(2,3,4): | |||||
| V821 Her | M | 3 × 10−6 | 13.0 | 600 | 752 |
| AI Vol(*) | M | 4.90 × 10−6 | 12.0 | 710 | 624 |
| AFGL 3068(*) | M | 1 × 10−5 | 13.5 | 980 | – |
References. (1)Ramstedt et al. (2009), (2)Schöier & Olofsson (2001), (3)González Delgado et al. (2003), (4)Danilovich et al. (2015), (5)Gaia Collaboration (2021); Bailer-Jones et al. (2021).
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