V1922 Aql | The light elements in the Table are for minina of the orbital variations. Also present are pulsations with P = 198d and an amplitude of 0.6mV. V1927 Aql | Period varies. Multiperiodic. V1928 Aql | VB A (9.8mV; B 10.2mV, 7", 104deg, 2013). The range in the Table is for combined brightness. V1936 Aql | A red star, despite the spectral type O4I in the literature. V1946 Aql | VB A (11.4mG; B 14.3mV, 6", 200deg, 2000). V1968 Aql | VB A (13.5mG; B 14.7mG, 3", 165deg, 2000); the range in the Table is influenced by the companion. V1971 Aql | MinII - MinI = 0.61P. V1977 Aql | P = 31.5d is superposed. V1992 Aql | VB A (8.3mG; B 11.4mG, 9", 72deg, 2000). The range in the Table is for combined brightness. V0778 CrA | P = 95d is superposed. V0782 CrA | VB B (A 14.0mV; AB 20", 355deg, 1991). The magnitude in maximum can be influenced by the companion. V0795 CrA | Blazhko effect? V0798 CrA | VB A (15.0mG; B 15.3mG, 7", 72deg, 2000); the range in the Table can be influenced by the companion. V0799 CrA | Blazhko effect? P varies? V0800 CrA | Blazhko effect? P varies? V0808 CrA | VB A (13.5mG; B 14.3mG, 12", 266deg, 2000); the range in the Table can be influenced by the companion. V2848 Cyg | The Table presents light elements for eclipses. Multiperiodic small-amplitude DSCT pulsations [82003]. V2850 Cyg | Multiperiodic, P2 = 0.11153d. V2855 Cyg | Multiperiodic, P2 = 0.0983128d. V2860 Cyg | Light elements for ELL type variability are presented in the Table. V2860 Cyg | Multiperiodic DSCTC oscillations with an amplitude of 0.02m are superposed. V2860 Cyg | The main harmonic: P = 0.058028d. V2863 Cyg | Multiperiodic. V2864 Cyg | VB A (13.7mG; B 15.4mG, 3", 99deg, 2000). V2871 Cyg | VB B (A 10.9mV; B 11.2mV, 17", 299deg, 2016); the range in the Table is for combined brightness. V2879 Cyg | VB A (12.5mG; B 13.3mG, 13", 213deg, 2000). V2883 Cyg | Crowded, several close companions. V2887 Cyg | VB A (15.9mG; B 17.0mG, 4", 50deg, 2000). V2888 Cyg | VB B (A 14.35mG, B 15.2mG; AB 13", 271deg, 2000). V0581 Dra | VB A (11.1mV; B 14.8mV, 1".1, 137deg, 2014; C 18.3mV, 6", 112deg, 2012). V1519 Her | VB A (B 5", 101, 2000). V0827 Lyr | VB A (B 5", 125deg, 2000); the range in the Table can be influenced by the companion. Type EW with a twice longer period is also possible. V0836 Lyr | Multiperiodic. P0 is presented in the Table; P1 = 0.090297d, P1/P0 = 0.7746; other periods. V0846 Lyr | VB B (A 14.9mG; B 15.3mG, 19", 146deg, 2000); the range in the Table can be influenced by the companion. V0868 Lyr | P varies? V0870 Lyr | Variations on the Palomar red plates: 16.3mR (1950 June 17) and 19.4mR (1987 June 21). V0870 Lyr | The Table presents light elements for EA variations during the high state. V0874 Lyr | The elements in the Table are for eclipses. ELL variations: P = 0.857724d, amplitude 0.02m. V0875 Lyr | VB A (B 9.1mV, 1".3, 126deg, 2015). The amplitude is for combined brightness. V3716 Oph | P = 56.3d is superposed. V3722 Oph | P = 48d is superposed. V3723 Oph | P = 47.3d is superposed. V3726 Oph | MinII - MinI = 0.42P. Apsidal motion. V0471 Pav | P = 68.6d is superposed. V0472 Pav | P = 43d is superposed. V0475 Pav | VB B (AB 7", 287deg, 2000). V0483 Pav | VB (15.22mG, 16.08mG, 3", 137deg, 2000); the range in the Table is for combined brightness. V0484 Pav | Possible secondary period 48d. V0491 Pav | P = 59.7d is superposed. V0494 Pav | Blazhko effect. V0500 Pav | P varies. V0537 Pav | Blazhko effect? V5954 Sgr | VB A (B 4", 22deg, 2000). The range is for combined brightness. V5960 Sgr | P = 142d is superposed. V5977 Sgr | P = 138d is superposed. V5980 Sgr | Porb = 1.2664d. V5985 Sgr | P = 97d is superposed. V5995 Sgr | P = 131d is superposed. V6099 Sgr | VB B (A 12mV; AB 4.4", 46deg, 2015). V6102 Sgr | P = 95.5d is superposed. V6109 Sgr | VB A (B 14m, 5", 138deg, 2000). V6125 Sgr | VB B (A 13m; AB 6", 54deg, 2000). V6173 Sgr | P = 163d is superposed. V6298 Sgr | P = 333d is superposed. V6318 Sgr | VB (NW); the SE component (NEXT STAR) 10", 123deg, 2000. V6319 Sgr | VB (SE); the NW component (PREVIOUS STAR) 10", 303deg, 2000. V6335 Sgr | VB A (B 14.36mG, 5", 2deg, 2000; C 14.39mG, 10", 258deg, 2000). V6361 Sgr | VB A (B 8", 135deg, 2000); the range in the Table can be influenced by the companion. V6386 Sgr | VB A (B 4", 326deg, 2000); the range in the Table is for combined brightness. Mira type is not excluded. V6434 Sgr | P = 71.7d is superposed. V6467 Sgr | P = 59d is superposed. V6474 Sgr | P = 119d is superposed. V6490 Sgr | VB A (12.8mG; B 14.3mG, 7", 87deg, 2000). V6495 Sgr | Long-term variations with a cycle about 750d are superposed. V6499 Sgr | VB A (B = EH Sgr, 12mV - 17mV, 47", 349deg, 2000). V6500 Sgr | VB A (9.5mV; B 9.8mV, 5", 161deg, 2000). The range in the Table is for combined brightness. V6501 Sgr | P = 64.7d is superposed. V6502 Sgr | P = 83.0d is also possible. V6508 Sgr | VB C (A 13.3mG; B 13.7mG, 29", 255deg, 2000; C 14.99mG, 11", 294deg, 2000; other companions). V6509 Sgr | Type EW with a twice longer period is also possible. V6515 Sgr | Blazhko effect? V6525 Sgr | Blazhko effect? V6554 Sgr | P1 is presented in the Table. P0 = 0.546995d; P1/P0 = 0.7457. V6555 Sgr | VB A (14.8mG; B 15.35mG, 17", 85deg, 2000; C 15.4mG, 18", 88deg, 2000). V6560 Sgr | Period varies. V0646 Sct | OH, H2O, SiO maser. V0661 Ser | H2O, OH maser. V0664 Ser | SiO, H2O maser. V0667 Ser | VB AB (10.2mV, 11.2mV, 3", 127deg, 2000). V0398 Tel | VB A (B 14.4mB, 10", 8deg, 2000). V0409 Tel | Type EW with a twice longer period is also possible. V0418 Tel | P varies. V0432 Tel | P = 52.3d is superposed. V0436 Tel | A twice longer period is not excluded. V0445 Tel | VB A (B 4", 322deg, 2000). V0466 Tel | VB A (B 15.1mG, 10", 91deg, 2000); the range in the Table can be influenced by the companion. V0470 Tel | P varies. V0475 Tel | O'Connell effect. V0478 Tel | Blazhko effect. V0487 Tel | Blazhko effect, P(Bl) = 52.8d. V0488 Tel | Blazhlo effect, P(Bl) = 37d. V0489 Tel | VB A (15.1mG; B 16.0mG, 5", 233deg, 2000). V0507 Tel | VB B (A 14.8mG; B 15.3mG, 3", 69deg, 2000). The range in the Table is for combined brightness. V0554 Vul | VB A (12.1mG; B 14.2mG, 11", 173deg, 2000). V0566 Vul | VB A (13.5mG; B 15.8mG, 8", 126deg, 2000); the range in the Table is influenced by the companion. V0571 Vul | Projected on the planetary nebula M27 = NGC 6853.