Terzan 8 / C1938-341 (Updated August 2014) RA: 19:41:44.41 DEC: -33:59:58.1 (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 19:41:55.13 -34 00 14.2 R0 0.6860 -- -- RR0 2 19:41:37.18 -34 03 17.6 R0 0.3920 -- -- RR1 3 19:41:31.96 -34 03 28.8 R0 0.6010 -- -- RR0 4 19:41:52.52 -33 59 16.8 R0 0.0616 -- -- SXPHE ======================================================================== Supplementary Notes The periods and classifications are from Salinas et al. (2005). The RA and dec were derived from the study by Salinas et al. (2012) and were provided by Salinas (2013, private communication). ======================================================================= Discovery of the variable stars in Terzan 8: V1-2 = Montegriffo's #1350 and #117 Montegriffo et al. (1998) announced 5 candidate variables: 117, 688, 1350, 1582 and 2784. They labelled them on an ID chart and published pixel positions (X,Y). Salinas et al. (2005) confirmed the variablility of #1350 and #117 and assigned the numbers V1 and 2. They also published x,y coordinates and a finding chart. However, the x,y coordinates they listed for V1 and V2 do not match the postions labelled on their chart. They are reversed. The numbering system used in ths catalogue corresponds to the positions on their chart. Montegriffo's candidate variable #2784 appears to be just outside the field of the finding chart of Salinas et al. Therefore it should still be considered a candidate variable. The other two candidates (#688 and #1582) are considered to be non-variable because Salinas et al. (2005) did not detect any variability. V3-4 Salinas et al. (2005) with x,y, coordinates and an ID chart =========================================================================== References Montegriffo, P., Bellazzini, M., Ferraro, F. R., Martins, D., Sarajedini, A., Fusi Pecci, F. 1998, MNRAS, 294, 315 Salinas, R., Catelan, M., Smith, H. A., Pritzl, B. J., Borissova, J. 2005, IBVS, 5640 Salinas, R., Jilkova, L., Carraro, G., Catelan, M., Amiga, P. 2012, MNRAS, 421, 960 =================================================================