**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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