# The Star Formation History of the Large Magellanic Cloud

## TL;DR

This study provides the first detailed, spatially-resolved history of star formation in the Large Magellanic Cloud, revealing key epochs, bursts, and a linked evolution with the Small Magellanic Cloud, based on extensive photometric data analysis.

## Contribution

It introduces a comprehensive, spatially-resolved star formation history of the LMC using the StarFISH software, revealing new insights into its temporal evolution and connection with the SMC.

## Key findings

- Star formation resumed about 5 Gyr ago after a quiescent period.
- Multiple recent peaks in star formation at 2 Gyr, 500 Myr, 100 Myr, and 12 Myr.
- Correlated star formation history between the LMC and SMC suggesting a joint evolutionary process.

## Abstract

We present the first-ever global, spatially-resolved reconstruction of the star formation history (SFH) of the Large Magellanic Cloud (LMC), based on the application of our StarFISH analysis software to the multiband photometry of twenty million of its stars from the Magellanic Clouds Photometric Survey. The general outlines of our results are consistent with previously published results: following an initial burst of star formation, there was a quiescent epoch from approximately 12 to 5 Gyr ago. Star formation then resumed and has proceeded until the current time at an average rate of roughly 0.2 solar masses/yr, with temporal variations at the factor-of-two level. The re-ignition of star formation about 5 Gyr ago, in both the LMC and SMC, is suggestive of a dramatic event at that time in the Magellanic system. Among the global variations in the recent star formation rate are peaks at roughly 2 Gyr, 500 Myr, 100 Myr and 12 Myr. The peaks at 500 Myr and 2 Gyr are nearly coincident with similar peaks in the SFH of the Small Magellanic Cloud, suggesting a joint history for these galaxies extending back at least several Gyr. The chemical enrichment history recovered from our StarFISH analysis is in broad agreement with that inferred from the LMC's star cluster population, although our constraints on the ancient chemical enrichment history are weak. We conclude from the concordance between the star formation and chemical enrichment histories of the field and cluster populations that the field and cluster star formation modes are tightly coupled.