NGC 6325 / C1714-237
RA: 17:17:59.21  DEC: -23:45:57.6 (J2000) 

(Most recent updates: 
Membership probability flag - 2024; Remaining data - April 2016)
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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
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ID       Position               Mem   Period <mag>  ampl  C Type  Notes/
         RA          Dec        Flag                              Remarks
=========================================================================
1        17:18:02.49 -23:45:44.8 m1  12.516  11.02  0.36  K CW
2        17:17:57.81 -23:46:36.4 m1  10.744  11.22  0.24  K CW 
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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 RA and dec for V1 and 2 are from Samus et al. (2021). The remaining
data are from the discovery paper by Matsunaga et al.  (2006).

The variable stars in NGC 6325 are also listed in the Moscow General 
Catalogue of Variable Stars (GCVS). A table listing their GCVS 
names was published in a paper by Samus et al.  (2021). 
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Discovery of the variable stars in NGC 6325

V1-2 
  Matsunaga et al. (2006) with RA and dec
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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 

Prudil Z., Arellano Ferro, A. 2024, MNRAS, 534, 3654

Samus, N. N., Pastukhova, E.N., Durlevich, O. V., Kazarovets, E. V.,
Kireeva, N. N. 2021, Per. Zvez., 41, No. 7

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