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Table 1
O-rich AGB stars in the sample.
| Name | RA | Dec | obs | D | Ṁ |
| (pc) | (M⊙ yr-1) | ||||
|
|
|||||
| IRC+10011 | 01 06 26.0 | +12 35 53.0 | 15 | 740 | 1.9E-5(1) |
| o Cet | 02 19 20.8 | −02 58 39.5 | 9 | 107 | 2.5E-7(1) |
| IK Tau | 03 53 28.9 | +11 24 21.7 | 15 | 260 | 4.5E-6(1) |
| R Dor | 04 36 45.6 | −62 04 37.8 | 9 | 59 | 2.0E-7(2) |
| TX Cam | 05 00 50.4 | +56 10 52.6 | 9 | 380 | 6.5E-6(1) |
| W Hya | 13 49 02.0 | −28 22 03.5 | 16 | 77 | 7.8E-8(1) |
| AFGL 5379 | 17 44 24.0 | −31 55 35.5 | 8 | 580 | 2.0E-4(3) |
| OH 26.5+0.6 | 18 37 32.5 | −05 23 59.2 | 8 | 1370 | 2.6E-4(3) |
| R Cas | 23 58 24.9 | +51 23 19.7 | 9 | 106 | 4.0E-7(1) |
Notes. Indicated is the number of frequency settings observed for each object.
References. The quoted distance and mass-loss rates are taken from (1) de Beck et al. (2010); (2) Maercker et al. (2009); and (3) Justtanont et al. (2006).
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