Table 5: Galactic O-rich AGB stars where the lithium line was detected.
    $v_{\rm exp}$(OH)   Period  
IRAS name Run (km s-1) Ref. (days) Ref.
01085+3022 3 13.0 3 560 1
02095-2355 1 $\dots$ $\dots$ $\dots$ $\dots$
04404-7427* 4 7.7 1 534 2
05027-2158 4 7.9 1 368 1
05559+3825 3 single peak 4 590 3
06300+6058 3 12.3 2 440 4
07222-2005* 4 8.2 1 1200 10
07304-2032 4 7.4 5 509 1
09429-2148 4 12.0 2 650 1
11081-4203 4 single peak 1 $\dots$ $\dots$
11525-5057 4 single peak 1 $\dots$ $\dots$
12377-6102* 4 20.4 1 $\dots$ $\dots$
14337-6215 4 19.7 9 $\dots$ $\dots$
15211-4254 4 11.0 1 $\dots$ $\dots$
15255+1944 1 7.4 2 425 1
15576-1212 4 9.9 2 415 1
16030-5156 4 single peak 1 $\dots$ $\dots$
16260+3454 1 12.3 2 475 1
18025-2113 1 10.6 1 $\dots$ $\dots$
18057-2616 1 18.7 1 $\dots$ $\dots$
18413+1354 2 14.7 4 590 3
18429-1721 1 6.9 1 $\dots$ $\dots$
19129+2803 2 single peak 1 420 10
19361-1658 2,3 7.5 1 $\dots$ $\dots$
20052+0554 2 15.6 12 450 3
* Tentative Li detection.
References for the OH expansion velocities:
1) te Lintel Hekkert et al. (1991); 2) te Lintel Hekkert et al. (1989); 3) Chengalur et al. (1993); 4) Slootmaker et al. (1985); 5) Sivagnanam et al. (1989); 6) Lewis et al. (1990); 7) Lewis et al. (1995); 8) Groenewegen et al. (2002) (from CO data); 9) Sevenster et al. (1997); 10) Groenewegen & de Jong (1998); 11) Nyman et al. (1992); 12) Lewis (1994) .
References for the periods:
1) Combined General Catalogue of Variable Stars (GCVS), Kholopov (1998); 2) Whitelock et al. (1994); 3) Jones et al. (1990); 4) Lockwood (1985); 5) Engels et al. (1983); 6) Nakashima et al. (2000); 7) Slootmaker et al. (1985); 8) Le Bertre (1993); 9) Herman & Habing (1985); 10) Jiménez-Esteban et al. (2006b).

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