Abstract:
We report an analysis of new
V and
I CCD time-series photometry of the
globular cluster NGC 6934. Through the Fourier decomposition of the RR Lyrae
light curves the mean values of [Fe/H] and the distance of the cluster were estimated; we found: [Fe/H]UV ES = −1.48 ± 0.14 and d = 16.03 ± 0.42 kpc, and
[Fe/H]UV ES
=
−
1
.43
±
0
.11 and
d = 15
.91
±
0
.39 kpc, from the calibrations of
RRab and RRc stars respectively. Independent distance estimations from SX Phe
and SR stars are also discussed. Individual absolute magnitudes, radii and masses
are also reported for RR Lyrae stars. We found 12 new variables: 4 RRab, 3 SX Phe,
2 W Virginis (CW) and 3 semi-regular (SR). The inter-mode or “either-or” region
in the instability strip is shared by the RRab and RRc stars. This characteristic,
observed only in some OoI clusters and never seen in an OoII, is discussed in terms
of mass distribution in the ZAHB.
