Table 2.
Basic properties of the sample stars.
| IRAS name | Identifier | Chem. | Puls. | Distance (Ref.) | υLSR (Ref.) | Ṁ (Ref.) |
|---|---|---|---|---|---|---|
| type | type | (kpc) | (km s−1) | (M⊙ yr−1) | ||
| AGB-stars |
||||||
| 01037+1219 | WX Psc | M | Mira | 0.74 (1) | 9.0 (13) | 4.0 × 10−5 (20) |
| 01246−3248 | R Scl | C | SRb | 0.27 (2) | −19.0 (14) | 1.0 × 10−6 (21) |
| 01304+6211 | OH 127.8 +0.0 | M | Mira | 2.10 (3) | −55.0 (13) | 5.0 × 10−5 (3) |
| 02168−0312 | o Cet | M | Mira | 0.09 (2) | 46.5 (15) | 2.5 × 10−7 (13) |
| 03507+1115 | IK Tau, NML Tau | M | Mira | 0.26 (4) | 34.0 (16) | 1.0 × 10−5 (20) |
| 04361−6210 | R Dor | M | SRb | 0.05 (2) | 7.0 (16) | 1.3 × 10−7 (20) |
| 04566+5606 | TX Cam | M | Mira | 0.39 (1) | 11.4 (16) | 1.0 × 10−5 (20) |
| 09425−6040 | … | C | Mira | 1.30 (5) | 15.0 (5) | 2.0 × 10−6 (5) |
| 09452+1330 | CW Leo | C | Mira | 0.12 (6) | −26.0 (15) | 1.5 × 10−5 (20) |
| 10131+3049 | RW LMi, CIT6 | C | SRa | 0.32 (7) | −1.8 (13) | 6.0 × 10−6 (20) |
| 10491−2059 | V Hya | C | SRa | 0.60 (7) | −16.0 (17) | 8.3 × 10−6 (7) |
| 13462−2807 | W Hya | M | Mira | 0.10 (2) | 40.5 (16) | 1.3 × 10−7 (22) |
| 15194−5115 | II Lup | C | Mira | 0.59 (7) | −5.5 (14) | 1.7 × 10−5 (14) |
| 16011+4722 | X Her | M | SRb | 0.14 (2) | −73.0 (15) | 1.5 × 10−7 (23) |
| 17411−3154 | AFGL 5379, OH 357.3−1.3 | M | Mira | 0.99 (1) | −21.2 (13) | 2.0 × 10−4 (8) |
| 18257−1000 | OH 21.5 +0.5 | M | Mira | 2.50 (8) | 115.0 (13) | 2.6 × 10−4 (8) |
| 18348−0526 | OH 26.5 +0.6 | M | Mira | 1.30 (9) | 29.0 (15) | 2.6 × 10−4 (8) |
| 18460−0254 | OH 30.1 −0.7 | M | Mira | 1.75 (8) | 100.0 (13) | 2.2 × 10−4 (8) |
| 18488−0107 | OH 32.0−0.5 | M | Mira | 3.90 (8) | 75.0 (13) | 3.6 × 10−4 (8) |
| 18498−0017 | OH 32.8 −0.3 | M | Mira | 4.30 (8) | 60.0 (13) | 3.1 × 10−4 (8) |
| 19039+0809 | R Aql | M | Mira | 0.42 (2) | 46.0 (18) | 3.5 × 10−6 (24) |
| 19067+0811 | OH 42.3−0.1 | M | Mira | 3.80 (8) | 60.0 (13) | 2.7 × 10−4 (12) |
| 19126−0708 | W Aql | S | Mira | 0.68 (10) | −27.5 (15) | 2.2 × 10−6 (12) |
| 19474−0744 | GY Aql | M | Mira | 0.22 (2) | 33.0 (18) | 6.0 × 10−6 (11) |
| 19486+3247 | χ Cyg | S | Mira | 0.18 (2) | 10.0 (15) | 3.8 × 10−7 (20) |
| 19550−0201 | RR Aql | M | Mira | 0.52 (2) | 28.0 (14) | 2.4 × 10−6 (14) |
| 20038−2722 | V1943 Sgr | M | SRb | 0.20 (2) | −15.0 (14) | 9.9 × 10−8 (14) |
| 20072+3116 | AFGL 2513 | C | Mira | 1.76 (7) | 17.8 (7) | 2.1 × 10−5 (7) |
| 20077−0625 | IRC −10 529, V1300 Aql | M | Mira | 0.66 (11) | −18.0 (14) | 3.0 × 10−5 (20 |
| 20248−2825 | T Mic | M | SRb | 0.21 (2) | 25.0 (19) | 8.0 × 10−8 (24) |
| 20396+4757 | V Cyg | C | Mira | 0.35 (2) | 15.0 (13) | 9.0 × 10−7 (20 |
| 21088+6817 | T Cep | M | Mira | 0.19 (2) | −2.0 (14) | 9.1 × 10−8 (14 |
| 21439−0226 | EP Aqr | M | SRb | 0.11 (2) | −34.0 (14) | 3.1 × 10−7 (13) |
| 22196−4612 | π Gru | S | SRb | 0.16 (2) | −12.0 (14) | 8.5 × 10−7 (13) |
| 23166+1655 | LL Peg, AFGL 3068 | C | Mira | 1.00 (7) | −31.0 (13) | 1.0 × 10−5 (20 |
| 23320+4316 | LP And, AFGL 3116 | C | Mira | 0.78 (7) | −17.0 (13) | 1.5 × 10−5 (20) |
| 23558+5106 | R Cas | M | Mira | 0.13 (2) | 25.0 (16) | 5.0 × 10−7 (20) |
| Red Super Giants |
||||||
| 05524+0723 | α Ori | M | SRc | 0.15 (2) | 3.5 (13) | 2.0 × 10−6 (25) |
| 07209−2540 | VY CMa | M | Lc | 1.17 (12) | 17.0 (15) | 3.0 × 10−4 (25) |
| … | NML Cyg | M | … | 1.61 (12) | −1.0 (15) | 8.7 × 10−5 (13) |
Notes. The sources are listed by the IRAS identifier. Column 1 lists the IRAS name, when available, and Col. 2 some common names. Column 3 gives the chemical type (M, S, or C), and Col. 4 the variability type. Columns 5–7 give the distance, velocity of the object (on the local standard of rest scale), and MLR, with the reference between parenthesis. References. (1) Olivier et al. (2001), (2) van Leeuwen (2007), (3) Lombaert et al. (2013), (4) Richards et al. (2012), (5) Molster et al. (2001), (6) Groenewegen et al. (2012), (7) Groenewegen et al. (2002), (8) Justtanont et al. (2006), (9) van Langevelde et al. (1990), (10) Groenewegen & de Jong (1998), (11) Loup et al. (1993), (12) Reid et al. (2014), (13) De Beck et al. (2010), (14) Danilovich et al. (2015), (15) de Vicente et al. (2016), (16) Danilovich et al. (2016), (17) Sahai et al. (2009), (18) Desmurs et al. (2014), (19) González Delgado et al. (2003), (20) Schöier et al. (2013), (21) Maercker et al. (2014), (22) Khouri et al. (2014a), (23) Olofsson et al. (2002), (24) Knapp & Morris (1985), (25) Smith et al. (2009).
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