# Variable stars in Palomar 13; an evaporating globular cluster

## TL;DR

This study provides detailed photometric analysis of Palomar 13, estimating its metallicity, distance, and age, and suggests the cluster is undergoing tidal disruption based on variable star analysis and Gaia data.

## Contribution

First detailed CCD photometry and variable star analysis of Palomar 13, revealing its metallicity, distance, age, and evidence of tidal stripping.

## Key findings

- Metallicity [Fe/H] = -1.65
- Distance approximately 23.67 kpc
- Cluster shows signs of tidal disruption

## Abstract

We present new CCD $VI$ photometry of the distant globular cluster Pal 13. Fourier decomposition of the light curves of the three cluster member RRab stars lead to estimations of [Fe/H]=-1.65, and a distance of 23.67$\pm$0.57 kpc. Light and colour near minimum phases for RRab stars leads to an estimate of $E(B-V)$=0.104 $\pm$ 0.001. A $V/(V-I)$ colour-magnitude diagram, built exclusively with likely star members, shows consistency with the above parameters and an age of 12 Gyrs. A search of variable stars in the field of view of our images revealed the variability of a red giant cluster member and of three probably non-member stars; two RRab stars and one W Virginis star or CW. The GAIA proper motions of member stars in Pal 13 show a significant scatter, consistent with the scenario of the cluster being tidally stripped.