Palomar 14 / C1608+150 (Updated September 2018) RA: 16:11:00.6 DEC: +14:57:28 (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 ========================================================================= No known variables. ========================================================================== Supplementary Notes Rosino & Ortolani (1985) noted that no variables had been found in this cluster, but pointed out that further observations would be required before reaching a definite conclusion. A CM diagram by Da Costa et al. (1982) indicated that the HB stars are red. This was confirmed by Dotter et al. (2008), Sollima et al. (2010) and Munoz et al. (2018) who all also showed that the cluster has a few blue stragglers. ============================================================== References Da Costa, G. S., Ortolani, S., Mould, J. 1982, ApJ, 257, 633 Dotter, A., Sarajedini, A., Yang, S.-C. 2008, AJ, 136, 1407 Munoz, R. R., Cote, P., Santana, F. A., Geha, M., Simon, J. D., Oyarzun, A., Stetson, P. B., Djorgovski, S. G. 2018, ApJ, 860, 66 Rosino, L. & Ortolani, S. 1985, Mem. Soc. Ast. It., 56, 113 Sollima, A., Martinez-Delgado, D., Vails-Gabaud, D., Penarrubia, J. 2010, ApJ, 726, 47 ===================================================================