A Synoptic View of the Magellanic Clouds: VMC, Gaia, and Beyond

TL;DR

This paper reviews recent advances in the study of the Magellanic Clouds, emphasizing observational data from VMC, Gaia, and upcoming surveys, to understand their role in galaxy evolution and distance measurement.

Contribution

It synthesizes current observational results and discusses future spectroscopic surveys to enhance understanding of the Magellanic Clouds and their significance in astrophysics.

Findings

Established the Magellanic Clouds as key laboratories for stellar and galaxy evolution.

Highlighted the importance of combining multi-wavelength data for comprehensive studies.

Outlined future survey plans to improve distance scale and galaxy interaction understanding.

Abstract

The year 2019 marked the quincentenary of the arrival in the southern hemisphere of Ferdinand Magellan, the namesake of the Magellanic Clouds, our nearest example of dwarf galaxies in the early stages of a minor merging event. These galaxies have been firmly established as laboratories for the study of variable stars, stellar evolution, and galaxy interaction, as well as being anchors for the extragalactic distance scale. The goal of this conference was to provide fertile ground for shaping future research related to the Magellanic Clouds by combining state-of-the-art results based on advanced observational programmes with discussions of the highly multiplexed wide-field spectroscopic surveys that will come online in the 2020s.