A Note on the Variability of V538 Cassiopeiae

TL;DR

This paper reports CCD observations of the star V538 Cassiopeiae over nine nights, finding no significant variability, contributing to the understanding of its stability.

Contribution

It provides new observational data on V538 Cassiopeiae, confirming its lack of significant variability over a three-week period.

Findings

No significant variations detected in V538 Cas.

Observations were made using the AAVSO Bright Star Monitor.

Data collected over nine nights.

Abstract

CCD observations of V538 Cas have been made on nine nights during three weeks using the AAVSO Bright Star Monitor. No significant variations were found.