RR Lyrae type stars, ST Boo and RR Leo: 2007 Observations and the preliminary results of the frequency analaysis

TL;DR

This study presents preliminary frequency analysis of pulsating stars ST Boo and RR Leo based on BVR light curves obtained in 2007, aiming to investigate their pulsation phenomena despite limited data.

Contribution

It provides initial frequency estimates for ST Boo and RR Leo using the Period04 software, contributing to understanding their pulsation behavior.

Findings

Possible frequencies identified for ST Boo and RR Leo

Preliminary insights into their pulsation phenomena

Data limitations acknowledged for definitive results

Abstract

We present BVR light curves of pulsating stars, ST Boo and RR Leo, obtained between March and September 2007 at the Ankara University Observatory (AUG) and the T\"{U}B{\.I}TAK National Observatory (TUG). Although these observational data are insufficient to obtain the reliable results for a frequency analysis of ST Boo and RR Leo stars, in this study, we tried to investigate the pulsation phenomena of these two stars, as an overview, using the Period04 software package. As preliminary results, we present the possible frequencies for ST Boo and RR Leo.