Bibcode
Dall'Ora, M.; Bono, G.; Storm, J.; Caputo, F.; Andreuzzi, G.; Marconi, G.; Monelli, M.; Ripepi, V.; Stetson, P. B.; Testa, V.
Bibliographical reference
Memorie della Società Astronomica Italiana, v.77, p.214 (2006)
Advertised on:
0
2006
Citations
7
Refereed citations
7
Description
We present new observational results on the RR Lyrae K-band
Period-Luminosity relation (PLK). Data on the Galactic globular clusters
NGC 3201 and NGC 4590 (M68), and on the Large Magellanic Cloud cluster
Reticulum are shown. We compare the observed slopes of the PLK relations
for these three clusters with those predicted by pulsational and
evolutionary models, finding a fair agreement. Trusting on this finding
we decided to adopt these theoretical calibrations to estimate the
distance to the target clusters, finding a good agreement with
optical-based RR Lyrae distances, but with a smaller formal scatter.