NGC 6273 / C1659-262 / Messier 19 (Updated September 2020) RA: 17:02:37.80 DEC: -26:16:04.7 (J2000) ============================================================ Bytes Format Explanation 1-8 A8 Star ID 10-32 A11,1x,A11 Position 34-35 A2 Units for position R0 denotes RA, DEC in the J2000 coordinates R5 denotes RA, DEC in the 1950 coordinates XA denotes X, Y in arcseconds XP denotes X, Y in pixels 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 Period ampl C Type Notes/ RA/X Dec/Y Units Remarks ========================================================================= 1 17:02:38.14 -26:15:11.8 R0 16.92 13.85 1.4 B CW 2 17:02:38.91 -26:13:57.4 R0 14.139 14.15 1.6 B CW Note 3 17:02:35.83 -26:16:06.5 R0 16.5 13.7 1.4 B CW 4 17:02:37.57 -26:16:31.6 R0 2.4326 14.75 1.5 B CW 5 17:02:32.25 -26:18:56.2 R0 0.5072 16.2 1.5 B RR0 6 17:03:03.46 -26:08:54.2 R0 0.5928 15.8 1.4 B RR0 f;Note 7 17:02:11.34 -26:13:51.1 R0 0.2444 14.53 0.45 B RR1 f;Note ========================================================================= Supplementary Notes All of the RA and dec in the above table are from Howard Bond (2020, private communication) based on Gaia DR2 astrometry. The remaining data are from Clement and Sawyer Hogg (1978), unless indicated otherwise on the Notes individual stars. ========================================================================= Notes on individual stars V2: Samus (1984) published observations of FK Oph and pointed out that FK Oph = V2 (NGC 6273) V6,V7: Howard Bond (2020, private communication) found that both V6 and V7 are non-members, based on Gaia DR2 astrometry. ============================================================== Discovery of the variable stars in M19: V1-V4, F1=V6 (=NSV 20887 in the Moscow GCVS) Sawyer (1943) with x,y positions and ID chart The number V6 was assigned by Clement & Sawyer Hogg (1978) V5 announced by Coutts et al. (1975) with x,y position and ID chart published by Clement & Sawyer Hogg (1978) V7= SVS 2155 Samus (1976) with ID chart and 1950 RA and dec The number V7 was assigned by Clement & Sawyer Hogg (1978) V7 is also V2135 Oph in the Moscow GCVS ================================================================= References Coutts, C. M., Sawyer Hogg, H., Thompson, D. C., 1975, Bull. AAS, 7, 536 Clement, C. C. & Sawyer Hogg, H. 1978, AJ, 83, 167 Samus, N. N. 1976, Astron. Tsirk., 900 Samus, N. N. 1984, IBVS, 2555 Sawyer, H. B. 1943, Publ. DDO, 1, 14 ======================================================================