UBVI Time-series Photometry of the Old LMC Globular Cluster Reticulum

Details UBVI Time-series Photometry of the Old LMC Globular Cluster Reticulum UBVI Time-series Photometry of the Old LMC Globular Cluster Reticulum

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004coast.145...24r&link_type=abstract

Communications in Asteroseismology, vol. 145, p. 24-27

Computer Science

1

Scientific paper

We present new UBVI CCD observations of the old LMC globular cluster RETICULUM. These data allowed us to re-determine periods and light curves and to identify 4 double mode RR Lyrae stars. A comparison with the theoretical instability strip in the M_V-log P plane shows good agreement between theory and observations when an apparent distance modulus of (m-M)=18.45+-0.12 mag (i.e.(m-M)_0=18.39+-0.12 mag) is assumed.

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