Table 1
Basic parameters of surveyed stars.
| Star | RA | Dec | υLSR | Distance | Ṁ | Teff | υ∞ | Ref. |
|---|---|---|---|---|---|---|---|---|
| (km s−1) | (pc) | (M⊙ yr−1) | (K) | (km s−1) | ||||
| 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 |
| U Hya | 10:37:33.27 | −13:23:04.4 | − 32 | 208 | 8.9 × 10−8 | 2400 | 6.5 | 1 |
| RV Aqr | 21:05:51.68 | −00:12:40.3 | 1 | 670 | 2.3 × 10−6 | 2200 | 15 | 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 |
| TX Cam | 05:00:50.39 | +56:10:52.6 | 11.4 | 380 | 4.0 × 10−6 | 2400 | 17.5 | 2 |
| NV Aur | 05:11:19.44 | +52:52:33.2 | 2 | 1200 | 2.5 × 10−5 | 2000 | 18 | 1 |
| BX Cam | 05:46:44.10 | +69:58:25.2 | −2 | 500 | 4.4 × 10−6 | 2800 | 19 | 1 |
| 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 |
| T Cep | 21:09:31.78 | +68:29:27.2 | −2 | 190 | 9.1 × 10−8 | 2400 | 5.5 | 1 |
| R Cas | 23:58:24.87 | +51:23:19.7 | 25 | 176 | 8.0 × 10−7 | 1800 | 10.5 | 2 |
| S-type stars | ||||||||
| T Cet | 00:21:46.27 | −20:03:28.9 | 22 | 240 | 6.0 × 10−8 | 2400 | 7 | 5 |
| R And | 00:24:01.95 | +38:34:37.4 | −16 | 350 | 5.3 × 10−7 | 1900 | 8 | 1 |
| V365 Cas | 01:00:53.16 | +56:36:45.2 | −2.1 | 625 | 3 × 10−8 | 2400 | 6.2 | 7 |
| S Cas | 01:19:41.99 | +72:36:40.8 | −30 | 570 | 2.8 × 10−6 | 1800 | 19 | 1 |
| W And | 02:17:32.96 | +44:18:17.8 | −35 | 450 | 2.8 × 10−7 | 2400 | 6 | 1 |
| T Cam | 04:40:08.88 | +66:08:48.7 | −11.7 | 540 | 1.0 × 10−7 | 2400 | 3.8 | 7 |
| DY Gem | 06:35:57.81 | +14:12:46.1 | −16.7 | 680 | 7.0 × 10−7 | 2400 | 8 | 7 |
| R Lyn | 07:01:18.01 | +55:19:49.8 | 16 | 850 | 3.3 × 10−7 | 2400 | 7.5 | 6 |
| R Gem | 07:07:21.27 | +22:42:12.7 | −60 | 820 | 4.3 × 10−7 | 2400 | 5 | 1 |
| AA Cam | 07:14:52.07 | +68:48:15.4 | −46.8 | 780 | 5.0 × 10−8 | 3000 | 5 | 5 |
| Y Lyn | 07:28:11.62 | +45:59:26.2 | −0.5 | 253 | 1.7 × 10−7 | 2400 | 8 | 1 |
| TT Cen | 13:19:35.02 | −60:46:46.3 | 4 | 1180 | 4.0 × 10−6 | 1900 | 20 | 5 |
| GI Lup | 15:06:16.31 | −41:28:13.8 | 6 | 690 | 5.5 × 10−7 | 2400 | 10 | 7 |
| ST Her | 15:50:46.63 | +48:28:58.9 | −4.5 | 293 | 1.3 × 10−7 | 2100 | 8.5 | 5 |
| ST Sco | 16:36:36.22 | −31:14:02.4 | −4.5 | 380 | 1.5 × 10−7 | 2400 | 5.5 | 7 |
| RT Sco | 17:03:32.55 | −36:55:13.7 | −47 | 400 | 4.5 × 10−7 | 2100 | 11 | 5 |
| TV Dra | 17:08:24.50 | +64:19:08.7 | 22 | 390 | 5 × 10−8 | 2400 | 4.7 | 7 |
| IRC-10401 | 18:10:24.82 | −10:34:16.1 | 19 | 585 | 2 × 10−6 | 1800 | 17 | 7a |
| ST Sgr | 19:01:29.20 | −12:45:34.0 | 55.7 | 540 | 2.0 × 10−7 | 2400 | 6 | 6 |
| S Lyr | 19:13:11.80 | +26:00:27.8 | 49 | 2000 | 3.5 × 10−6 | 1800 | 13 | 5 |
| W Aql | 19:15:23.35 | −07:02:50.4 | −23 | 395 | 3.0 × 10−6 | 2300 | 16.5 | 4 |
| EP Vul | 19:33:17.84 | +23:39:19.6 | 0 | 510 | 2.3 × 10−7 | 2800 | 6 | 5 |
| R Cyg | 19:36:49.38 | +50:11:59.5 | −17 | 690 | 9.5 × 10−7 | 2600 | 9 | 1 |
| AFGL 2425 | 19:39:00.74 | −16:51:56.5 | 57 | 610 | 3.0 × 10−7 | 1800 | 8.7 | 7 |
| CSS2 41 | 19:39:07.77 | +29:02:38.6 | 21.5 | 880 | 5.8 × 10−7 | 1800 | 17 | 7 |
| χ Cyg | 19:50:33.92 | +32:54:50.6 | 9 | 150 | 7.9 × 10−7 | 2600 | 8.5 | 8 |
| AA Cyg | 20:04:27.61 | +36:49:00.5 | 27.5 | 480 | 2.9 × 10−7 | 2400 | 4.5 | 7 |
| DK Vul | 20:06:33.96 | +24:25:60.0 | −15 | 750 | 2.0 × 10−7 | 2900 | 4.5 | 5 |
| RZ Sgr | 20:15:28.41 | −44:24:37.5 | −31 | 730 | 3.0 × 10−6 | 2400 | 9 | 6 |
| AD Cyg | 20:31:36.51 | +32:33:52.4 | 21 | 980 | 2.1 × 10−7 | 1800 | 8 | 7 |
| RZ Peg | 22:05:52.97 | +33:30:24.8 | −23.4 | 970 | 4.6 × 10−7 | 2400 | 12.6 | 6 |
| RX Lac | 22:49:56.90 | +41:03:04.3 | −15.4 | 310 | 8 × 10−8 | 2400 | 6.5 | 7 |
| V386 Cep | 22:53:12.33 | +61:17:00.4 | −51.8 | 470 | 2.0 × 10−7 | 1800 | 16 | 7 |
| WY Cas | 23:58:01.31 | +56:29:13.5 | 7 | 600 | 1.1 × 10−6 | 2200 | 13.5 | 6 |
Notes. Upper section contains APEX sulphur survey sources, lower section details S-star survey, omitting duplicates. References give details of mass-loss rate, Ṁ, stellar effective temperature, Teff, distances, and dust properties. (a)Indicates that stellar properties were updated in this work.
References: (1) Danilovich et al. (2015); (2) Maercker et al. (2016); (3) Khouri et al. (2014a) and Danilovich et al. (2016); (4) Danilovich et al. (2014) and Ramstedt et al. (2017); (5) Ramstedt & Olofsson (2014); (6) Schöier et al. (2013); (7) Ramstedt et al. (2009); (8) Schöier et al. (2011).
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.