Among over 200 000 Galactic bulge variable stars in the public domain Optical Gravitational Lensing Experiment (OGLE) catalogue, we found over 15 000 red giant variables following two well-defined period-amplitude relations. The periods are in the range 10 < P < 100 d, and amplitudes in the range 0.005 < A < 0.13 mag in the I band. The variables cover a broad range of reddening-corrected colours, 1 < (V -I) 0 < 5, and a fairly narrow range of extinction-corrected apparent magnitudes, 10.5 < I 0 < 13. A subset of variables (type A) has an rms scatter of only 0.44 mag. The average magnitudes for these stars are well correlated with the Galactic longitude, and vary from I k,0 = 11.82 for l = + 8 to I k,0 = 12.07 for l = -5 , clearly indicating that they are located in the Galactic bar. Most variables have several oscillation periods.
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Wray et al. (2004) studied this question.
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