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Table 1

List of the observed OH/IR stars and possible detections of crystalline olivine spectral bands.

Source name IRAS # (Ṁ10-5 M/yr) 11.3 μm 33.6 μm 69.0 μm P(days) L(L)

OH 32.8-0.3 18498−0017 1 16 (1) + + + 1539 23 100
OH 21.5+0.5 18257−1000 2 26 (2) ? + + 1785 72 100−96 900
OH 30.1-0.7 18460−0254 3 18 (3) + + + 2013
OH 26.5+0.6 18348−0526 4 3.2 (4) + + + 1570 39 362
OH 127.8+0.0 01304+6211 5 9.2 (3) + + 1525 38 012
AFGL 2403 19283+1944 6 1.7 (5) + + + 1574
IRAS 21554 21554+6204 7 1.5 (5) ? + + 4984
AFGL 5379 17411−3154 8 9.8 (3) + + 1440 35 484
OH 104.91+2.4 22177+5936 9 5.6 (6) + 1620 40 871
AFGL 4259 20043+2653 10 +
IRAS 17010 17010−3840 11 + +
RAFGL 2374 19192+0922 12 0.46 (5) ? + 534 4300
WX Psc 01037+1219 13 1.7 (3) ? + 660 13 914
IRC+50137 05073+52 48 14 0.6 (7) ? + 635 13 284

Reference. References for the mass loss rates: (1) Groenewegen (1994); (2) Justtanont et al. (2006); (3) Justtanont et al. (2013); (4) Justtanont et al. (1996); (5) De Beck et al. (2010); (6) Riechers et al. (2005); (7) Justtanont & Tielens (1992). References for the periods and luminosities are van Langevelde et al. (1990) and De Beck et al. (2010) and references therein.

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