NGC 6356 / C1720-177 RA: 17:23:34.93 DEC: -17:48:46.9 (J2000) (Most recent updates: Membership probability flag - 2024; Remaining data - July 2013) ============================================================ Bytes Format Explanation 1-8 A8 Star ID 10-32 A11,1x,A11 Position 34-35 A2 Membership probability flag based on data published by Prudil & Arellano Ferro (2024) m1: prob >=0.85; m2: prob >=0.7 and <0.85; m3: prob >= 0.5 and <0.7; f: prob <0.5 u: no data available 37-44 F8.4 Period (days) 46-51 F6.3 Mean magnitude (or maximum magnitude if "max" is indicated in the remarks column) 53-57 F5.3 Light amplitude (range of variability) 59 A1 Colour for mean magnitude and amplitude e.g. B, V, R, I, J, K or P (for photographic). 61-65 A5 Type of variable (draft 2006 GCVS classifications) CST denotes non variable stars previously designated as variables 67-80 A19 Notes and Remarks (f denotes field star) "--" or "----" indicates no data available ========================================================================= ID Position Mem Period ampl C Type Notes/ RA Dec Flag Remarks ========================================================================= 1 17:23:33.72 -17:49:14.8 m2 230.6 17.35 1.7 B M 2 17:23:42.12 -17:50:41.3 m1 ---- 17.6 0.8 B Lb 3 17:23:33.30 -17:48:07.4 m1 220.0 16.9 2.8 B M mem 4 17:23:48.00 -17:48:04.5 m1 207.3 17.35 2.3 B M f? 5 17:23:17.06 -17:46:24.5 m1 219.8 17.55 1.9 B M 6 17:22:54.71 -17:47:00.2 u 189.8 17.2 2.6 B M f? 7 17:23:34.51 -17:49:13.0 f ---- 15.5 0.2 V Lb 8 17:23:32.07 -17:47:59.2 m1 ---- 15.8 0.4 V Lb 9 17:23:32.47 -17:48:12.7 m1 ---- 15.6 0.4 V Lb 10 17:23:32.09 -17:49:15.3 m2 ---- 15.65 0.1 V Lb ================================================================== Supplementary Notes The RA and dec for the variables are from Samus et al. (2009). V1-6: Periods, magnitudes, amplitudes, variability types for V1-6 are from Clement & Sawyer Hogg (1977) Membership status for V3 is based on a radial velocity study by Feast (1972). Possible field status for V4 is from Lloyd Evans & Menzies (1973) and for V6 from Clement & Sawyer Hogg (1977). With a distance of 9.8 arcmin from the cluster centre, V6 is outside the tidal radius of 9.3 arcmin (Harris 1996 - 2010 update). V7-10: Magnitudes and amplitudes for V7-10 are from Lloyd Evans & Menzies (1977). They classified these stars as red variables. Since the GCVS does not use this term, we have classified them as Lb. ================================================================ Discovery of the variable stars in NGC 6356: V1-5, F1=V6 Sawyer, JRASC 47, 229 (1953) with x,y positions and ID chart for V1-5 Sawyer Hogg (1973) assigned the number V6 to F1 in her 3rd catalogue and an ID chart for V6 was published by Clement & Sawyer Hogg (1977). In the Moscow GCVS, V5 and V6 are listed as V2009 and V1995 Oph respectively.. V7-10 Lloyd Evans & Menzies (1973) who identify them as stars 34, 72, 30 and 46 of Sandage & Wallerstein (1960 - see Fig 2) Sandage & Wallerstein (1960) also labelled V1 and V3 in Fig.2 and V2, V4 and V5 in Fig. 1 of their paper. ================================================================ References Clement, C. C. & Sawyer Hogg, H. 1977, AJ, 82, 968 Feast, M. W. 1972, QJRAS, 13, 191 Lloyd Evans, T. & Menzies, J. W. 1973, IAU Colloq. No. 21, Variable Stars in Globular Clusters and in Related Systems, 151 Lloyd Evans, T. & Menzies, J. W. 1977, MNRAS, 178, 163 Prudil Z., Arellano Ferro, A. 2024, MNRAS, 534, 3654 Samus, N. N., Kazarovets, E. V., Pastukhova, E. N., Tsvetkova, T. M., Durlevich, O. V. 2009, PASP, 121, 1378 Sandage, A. R. & Wallerstein, G. 1960, ApJ, 131, 598 Sawyer, H. B. 1953, JRASC, 47, 229 Sawyer Hogg, H. 1973, Publ. DDO, 3, No. 6 =====================================================================