G. Piotto et al., Hubble Space Telescope observations of Galactic globular cluster cores. II. NGC 6273 and the problem of horizontal-branch gaps, ASTRONOM J, 118(4), 1999, pp. 1727-1737
We present observations of the center of the Galactic globular cluster NGC
6273, obtained with the Hubble Space Telescope Wide Field Planetary Camera
2 as part of the snapshot program GO-7470. A BV color-magnitude diagram (CM
D) for similar to 28,000 stars is presented and discussed. The most promine
nt feature of the CMD, identified for the first time in this paper, is the
extended horizontal-branch blue tail (EBT) with a clear double-peaked distr
ibution and a significant gap. The EBT of NGC 6273 is compared with the EBT
s of seven other globular clusters for which we have a CMD in the same phot
ometric system. From this comparison, we conclude that all the globular clu
sters in our sample with an EBT show at least one gap along the horizontal
branch, which could have similar origins. A comparison with theoretical mod
els suggests that at least some of these gaps may be occurring at a particu
lar value of the stellar mass, common to a number of different clusters. Fr
om the CMD of NGC 6273 we obtain a distance modulus (m - M)(v) = 16.27 +/-
0.20. We also estimate an average reddening E(B-V) = 0.47 +/- 0.03, though
the CMD is strongly affected by differential reddening, with the relative r
eddening spanning a Delta E(B-V) similar to 0.2 mag in the WFPC2 held. A lu
minosity function for the evolved stars in NGC 6273 is also presented and c
ompared with the most recent evolutionary models.