INT monitoring survey of Local Group dwarf galaxies: star formation history and chemical enrichment

TL;DR

This survey of 55 Local Group dwarf galaxies using the INT telescope aims to understand their star formation history and chemical enrichment by studying variable stars like AGB and RSG stars.

Contribution

It provides new observational data on LPV stars in dwarf galaxies, enhancing understanding of their evolution and structure formation.

Findings

Identification of LPV stars in 55 dwarf galaxies

Insights into star formation history and chemical enrichment

Data on the radial distribution and mass-loss rates of AGB stars

Abstract

The Local Group (LG) hosts many dwarf galaxies with diverse physical characteristics in terms of morphology, mass, star formation, and metallicity. To this end, LG can offer a unique site to tackle questions about the formation and evolution of galaxies by providing detailed information. While large telescopes are often the first choices for such studies, small telescope surveys that perform dedicated observations are still important, particularly in studying bright objects in the nearby universe. In this regard, we conducted a nine epoch survey of 55 dwarf galaxies called the Local Group dwarf galaxies survey using the 2.5m Isaac Newton Telescope (INT) in La Palma to identify Long-Period Variable (LPV) stars, namely Asymptotic Giant Branch (AGB) and Red Super Giant (RSG) stars. AGB stars formed at different times and studying their radial distribution and mass-loss rate can shed light on the structure formation in galaxies. To further investigate the evolutionary path of these galaxies, we construct their star formation history (SFH) using the LPV stars, which are at the final stages of their evolution and therefore experience brightness fluctuations on the timescales between hundred to thousand days. In this paper, we present some of the results of the Local Group dwarf galaxies survey.