Table 1.
Forty-two sources observed with the ACA by spectral type and variability type listed in ascending mass-loss-rate order.
| Source | Variability | Ṁ(a) | v∞(a) | D | DGaia |
|---|---|---|---|---|---|
| type | [M⊙ yr−1] | [km s−1] | [pc] | [pc] | |
| M-type semi-regular and irregular stars: | |||||
| L2 Pup | SRb | 2 × 10−8 | 2.3 | 85 | 140 |
| W Hya | SRa | 8 × 10−8 | 6.5 | 65 | 160 |
| T Mic | SRb | 8 × 10−8 | 4.8 | 130 | 190 |
| Y Scl | SRb | 1.3 × 10−7 | 5.2 | 330 | 310 |
| V1943 Sgr | Lb | 1.3 × 10−7 | 5.4 | 150 | 665 |
| BK Vir | SRb | 1.5 × 10−7 | 4.0 | 190 | 235 |
| V Tel | SRb | 2 × 10−7 | 6.8 | 290 | 400 |
| SU Vel | SRb | 2 × 10−7 | 5.5 | 250 | 290 |
| UY Cet | SRb | 2.5 × 10−7 | 6.0 | 300 | 320 |
| SV Aqr | Lb | 3 × 10−7 | 8.0 | 470 | 390 |
| SW Vir | SRb | 4 × 10−7 | 7.5 | 120 | 300 |
| CW Cnc | Lb | 5 × 10−7 | 8.5 | 280 | 210 |
| RT Vir | SRb | 5 × 10−7 | 7.8 | 170 | 490 |
| R Crt | SRb | 8 × 10−7 | 10.6 | 170 | 240 |
| M-type Mira stars: | |||||
| R Leo | M | 2 × 10−7 | 6.0 | 130 | 70 |
| R Hya | M | 3 × 10−7 | 7.0 | 150 | 225 |
| R Hor | M | 5.9 × 10−7 | 4.0 | 310 | 310 |
| RR Aql | M | 2.4 × 10−6 | 9.0 | 530 | 320 |
| IRC-10529 | M | 2.5 × 10−6 | 12.0 | 270 | – |
| WX Psc | M | 1.1 × 10−5 | 19.3 | 600 | – |
| IRC+10365 | M | 3 × 10−5 | 16.2 | 750 | 360 |
| C-type semi-regular and irregular stars: | |||||
| TW Oph | SRb | 5 × 10−8 | 7.5 | 280 (b) | 590 |
| NP Pup | Lb | 6.5 × 10−8 | 9.5 | 420 (b) | 470 |
| TW Hor | SRb | 9 × 10−8 | 5.5 | 400 (b) | 420 |
| T Ind | SRb | 9 × 10−8 | 6.0 | 570 (b) | 610 |
| RT Cap | SRb | 1 × 10−7 | 8.0 | 450 (c) | 430 |
| AQ Sgr | SRb | 2.5 × 10−7 | 10.0 | 420 (d) | 560 |
| U Hya | SRb | 1.2 × 10−7 | 7.0 | 160 (b) | 170 |
| W Ori | SRb | 1.4 × 10−7 | 11.0 | 220 (b) | 1010 |
| V Aql | SRb | 1.5 × 10−7 | 8.5 | 370 (b) | 400 |
| Y Pav | SRb | 1.6 × 10−7 | 8.0 | 360 (c) | – |
| X Vel | SR | 1.8 × 10−7 | 10.0 | 310 (c) | 640 |
| Y Hya | SRb | 1.9 × 10−7 | 9.0 | 350 (b) | 475 |
| SS Vir | SRa | 2 × 10−7 | 12.5 | 540 (c) | 670 |
| W CMa | Lb | 3 × 10−7 | 10.5 | 450 (d) | 555 |
| C-type Mira stars: | |||||
| R Lep | M | 7 × 10−7 | 18.0 | 250 (b) | 420 |
| CZ Hya | M | 9 × 10−7 | 12.0 | 960 (c) | 3300 |
| R For | M | 1.1 × 10−6 | 16.5 | 610 (c) | 630 |
| R Vol | M | 1.7 × 10−6 | 18.0 | 730 (c) | 840 |
| RV Aqr | M | 2 × 10−6 | 16.0 | 670 (c) | 860 |
| V688 Mon | M | 6.1 × 10−6 | 13.5 | 1770 (e) | 500 |
| V1259 Ori | M | 8.8 × 10−6 | 16.0 | 1600 (e) | – |
Notes. The columns give wind properties (mass-loss rate, Ṁ, and final expansion velocity, v∞), and preliminary distance, D, from previous publications (see text for details). The final column gives the distances from Gaia data release 2 (Bailer-Jones et al. 2018) for comparison purposes (see also Fig. 2).
Period-luminosity relation (Groenewegen & Whitelock 1996).
Adopted from Menzies et al. (2006).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.