Table 1
Basic parameters of surveyed stars.
| Star | RA | Dec | υ LSR | Distance | Ṁ | T eff | υ ∞ | Ref. |
| [km s-1] | [pc] | [M⊙ yr-1] | [K] | [km s-1] | ||||
|
|
||||||||
| M-type stars | ||||||||
| R Hor | 02:53:52.77 | −49:53:22.7 | 37 | 310 | 5.9 × 10-7 | 2200 | 4 | 1 |
| IK Tau | 03:53:28.87 | +11:24:21.7 | 34 | 265 | 5.0 × 10-6 | 2100 | 17.5 | 2 |
| GX Mon | 06:52:46.91 | +08:25:19.0 | −9 | 550 | 8.4 × 10-6 | 2600 | 19 | 1 |
| W Hya | 13:49:02.00 | −28:22:03.5 | 40.5 | 78 | 1.0 × 10-7 | 2500 | 7.5 | 3 |
| RR Aql | 19:57:36.06 | −01:53:11.3 | 28 | 530 | 2.3 × 10-6 | 2000 | 9 | 1 |
| V1943 Sgr | 20:06:55.24 | −27:13:29.8 | −15 | 200 | 9.9 × 10-8 | 2200 | 6.5 | 1 |
| V1300 Aql | 20:10:27.87 | −06:16:13.6 | −18 | 620 | 1.0 × 10-5 | 2000 | 14 | 1 |
| V1111 Oph | 18:37:19.26 | +10:25:42.2 | −32 | 750 | 1.2 × 10-5 | 2000 | 17 | 1 |
| WX Psc | 01:06:25.98 | +12:35:53.1 | 9.5 | 700 | 4.0 × 10-5 | 1800 | 19 | 5 |
| IRC-30398 | 18:59:13.85 | −29:50:20.4 | −6.5 | 550 | 8.0 × 10-6 | 1800 | 16 | 5 |
| S-type stars | ||||||||
| T Cet | 00:21:46.27 | −20:03:28.9 | 22 | 240 | 6.0 × 10-8 | 2400 | 7 | 5 |
| TT Cen | 13:19:35.02 | −60:46:46.3 | 4 | 880 | 4.0 × 10-6 | 1900 | 20 | 5 |
| W Aql | 19:15:23.35 | −07:02:50.4 | −23 | 395 | 4.0 × 10-6 | 2300 | 16.5 | 4 |
| RZ Sgr | 20:15:28.41 | −44:24:37.5 | −31 | 730 | 3.0 × 10-6 | 2400 | 9 | 6 |
| Carbon stars | ||||||||
| R Lep | 04:59:36.35 | −14:48:22.5 | 11 | 432 | 8.7 × 10-7 | 2200 | 18 | 1 |
| V1259 Ori | 06:03:59.84 | +07:25:54.4 | 42 | 1600 | 8.8 × 10-6 | 2200 | 16 | 1 |
| AI Vol | 07:45:02.80 | −71:19:43.2 | −39 | 710 | 4.9 × 10-6 | 2100 | 12 | 1 |
| X TrA | 15:14:19.18 | −70:04:46.1 | −2 | 360 | 1.9 × 10-7 | 2200 | 6.5 | 1 |
| II Lup | 15:23:04.91 | −51:25:59.0 | −15.5 | 500 | 1.7 × 10-5 | 2400 | 21.5 | 1 |
| V821 Her | 18:41:54.39 | +17:41:08.5 | −0.5 | 600 | 3.0 × 10-6 | 2200 | 13.5 | 1 |
| RV Aqr | 21:05:51.68 | −00:12:40.3 | 1 | 670 | 2.3 × 10-6 | 2200 | 15 | 1 |
Notes. References give details of mass-loss rate, Ṁ, stellar effective temperature, Teff, and distances. (1) Danilovich et al. (2015); (2) Maercker et al. (2016); (3) Khouri et al. (2014) and Danilovich et al. (2016); (4) Danilovich et al. (2014); (5) Ramstedt & Olofsson (2014); (6) Schöier et al. (2013).
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