1 Near WR 107a (SMSNPL18, Shara et al., 1999AJ....118..390S). 
 2 Identical with [DSH99]454-20 (Dufton et al., 1999, Cat. <J/A+AS/139/231>) and
 2  very probably with PM 1-130 (Preite-Martinez, 1988A&AS...76..317P) = RPZM 4.
 3 Identical with V2400 Oph. 
 4 Near 393-92. 
 5 Near 393-39. 
 6 Identical with Terz V348 (Terzan et al., 1982, Cat. <J/A+AS/49/715>). 
 7 Near 455-255. 
 8 Near 455-254. 
 9 Identical with Terz V2687 (Terzan & Gosset, 1991, Cat. <J/A+AS/90/451>).
10 Near Ve 2-50 (Velge, 1957ApJ...126..302V). 
11 Near V703 Sco. 
12 Probably identical with [GWC93]38 (Gray et al., 1993MNRAS.264..678G). 
13 Identical with [RHI84]10-424 (Raharto et al., 1984AnTok..19..469R). 
14 Near/in open cluster Collinder 347 (OCl-1039, C 1743-292). 
15 Near/in open cluster Collinder 347 (OCl-1039, C 1743-292). 
16 Possibly identical with radio source GRS 000.60-00.10. 
17 Identical with [RHI84]10-788 (Raharto et al., 1984AnTok..19..469R). 
18 Near cluster of stars NGC 6451 (C 1747-302). 
19 Possibly identical with infrared source HFE 40 
19  (Hoffmann et al., 1971ApJ...170L..89H). 
20 Very probably identical with post-AGB star GLMP 676 
20  (Garcia-Lario et al., 1997, Cat. <J/A+AS/126/479>). 
21 Identical with V589 Sgr. 
22 H-alpha variable. 
23 Near 521-119. 
24 Identical with He 2-294, which was misclassified as PN in Kohoutek (2001, 
24  Cat. <IV/24>), Table 3. 
25 Near Ve 2-57 (Velge, 1957ApJ...126..302V).
31 He 3-1339. 
32 He 3-1444,WRA 15-1745. 
33 He 3-1498. 
34 MAC 3-608. 
35 LSS 4557. 
36 WRA 16-355. 
37 Ve 1-16, near 521-118. 
38 He 3-1551. 
39 MAC 3-573; in Trumpler 27 (OCl-1021, C1732-334). 
41 394-48. Uncertain identification in van der Hucht et al. (1981, 
41  Cat. <III/215>). 
42 394-57; faint star with medium H-alpha em. line visible, we agree with Henize
42  (1976ApJS...30..491H) that it is a nova which will be dealt with in a 
42  separate paper. 
43 521-98. 
44 Star to E disturbs. 
45 Ve 2-38. 
46 He 3-1539. No H-alpha em.line visible. 
47 The visible em.line is not H-alpha. 
48 The double star having NW and SE components in the centre is obviously 
48  LKH 346 and is identical with Th 27-4 (The, 1961CoBos..10....1T). The two 
48  components have a distance of about 4.4"; the cross in the finding chart 
48  show their mean position. The coordinates given above differ from those of 
48  SIMBAD. KW 2 is a new H-alpha em.line star (see Table 1). 
49 No H-alpha em. line was visible on three plates taken in 1967 Aug.; the 
49  continuum was fainter than that of the star situated 1.6" to SW. On the 
49  direct plate taken in 1980 May the variable appeared brighter than this 
49  star. The identification given by Lundstrom & Stenholm (1978IBVS.1393....1L)
49  was used. 
50 LKH 102 (Herbig, 1957ApJ...125..654H). 
51 Star to N disturbs.