NGC 6325 / C1714-237 (Updated April 2016) RA: 17:17:59.21 DEC: -23:45:57.6 (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 17:18:02.5 -23:45:45 R0 12.516 11.02 0.36 K CW 2 17:17:57.8 -23:46:36 R0 10.744 11.22 0.24 K CW =============================================================== Supplementary Notes This cluster is embedded in a crowded field in the Galactic bulge. According to the 2010 version of the Harris (1996) catalogue, it is a core collapsed cluster with [Fe/H] = -1.25. BVI photometry by Ortolani et al. (2003) shows a prominent blue HB with evidence for a blue tail. The data for V1 and 2 are from the discovery paper by Matsunaga et al. (2006). =================================================================== Discovery of the variable stars in NGC 6325 V1-2 Matsunaga et al. (2006) with RA and dec =================================================================== References Harris, W. E. 1996, AJ, 112, 1487 Matsunaga, N., Fukushi, H., Nakada, Y., Tanabe, T., Feast, M. W., Menzies, J. W., Ita, Y. and 7 coauthors, 2006, MNRAS, 370, 1979 Ortolani, S., Bica, E., Barbuy, B. 2003, A&A, 402, 565 =================================================================