S. Ortolani et al., NTT VI PHOTOMETRY OF THE METAL-RICH AND OBSCURED BULGE GLOBULAR-CLUSTER TERZAN-5, Astronomy and astrophysics, 308(3), 1996, pp. 733-737
We study the metal-rich bulge globular cluster Terzan 5 by means of VI
colour-magnitude diagrams, with images obtained under exceptional see
ing conditions (0.34 ''-0.50 ''). Differential reddening is important
across the cluster. We derive a reddening of E(B - V) = 2.49 and a dis
tance from the Sun d. = 5.6 kpc, closer than previous estimates. Based
on the red giant branch curvature, we derive a metallicity somewhat h
igher than that of NGC 6553, probably solar.