The star formation history of the Magellanic Clouds derived from long-period variable star counts
Sara Rezaei kh. (IPM, Iran), Atefeh Javadi (IPM), Habib Khosroshahi, (IPM), Jacco Th. van Loon (Keele University, UK)

TL;DR
This study reconstructs the star formation history of the Magellanic Clouds using long-period variable stars, revealing distinct epochs and suggesting different formation scenarios for the LMC and SMC.
Contribution
It introduces a novel method of deriving star formation history from long-period variable star counts in the Magellanic Clouds.
Findings
Identified a 10-Gyr old star formation epoch in the LMC.
Detected a secondary star formation episode in the LMC bar 3-0.5 Gyr ago.
Found two distinct star formation epochs in the SMC, one 6 Gyr ago and another 0.7 Gyr ago.
Abstract
We present the first reconstruction of the star formation history (SFH) of the Large and Small Magellanic Clouds (LMC and SMC) using Long Period Variable stars. These cool evolved stars reach their peak luminosity in the near-infrared; thus, their K-band magnitudes can be used to derive their birth mass and age, and hence the SFH can be obtained. In the LMC, we found a 10-Gyr old single star formation epoch at a rate of M yr, followed by a relatively continuous SFR of M yr, globally. In the core of the LMC (LMC bar), a secondary, distinct episode is seen, starting 3 Gyr ago and lasting until Gyr ago. In the SMC, two formation epochs are seen, one Gyr ago at a rate of M yr and another only Gyr ago at a rate of M yr. The latter is also discernible in the LMC and…
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