KMHK 1762: Another star cluster in the Large Magellanic Cloud age gap
arXiv:2207.09478 · doi:10.1051/0004-6361/202243993
Abstract
The star cluster (SC) age distribution of the Large Magellanic Cloud (LMC) exhibits a gap from 4 to 10 Gyr ago, with an almost total absence of SCs. Within this age gap, only two confirmed SCs have been identified hitherto. Nonetheless, the star field counterpart does not show the same characteristics, making the LMC a peculiar galaxy where star formation history and cluster formation history appear to differ significantly. We re-analyzed the color-magnitude diagram (CMD) of the KMHK 1762 SC by using the deep optical photometry provided by the "Yes, Magellanic Clouds Again" survey, to robustly assess its age. First, we partially removed foreground and/or field stars by means of parallaxes and proper motions obtained from the {\it Gaia} Early Data Release 3. Then, we applied the Automated Stellar Cluster Analysis package to the cleaned photometric catalogue to identify the isochrone that best matches the CMD of KMHK 1762. The estimated age of KMHK 1762 is dex (5.5 Gyr), that is more than 2 Gyr older than the previous estimation which was obtained with shallower photometry. This value makes KMHK 1762 the third confirmed age gap SC of the LMC. The physical existence of a quiescent period of the LMC SC formation is questioned. We suggest it can be the result of an observational bias, originated by the combination of shallow photometry and limited investigation of the LMC periphery.
arXiv comment6 pages, 4 figures. Accepted for publication in A&A Letter
References in corpus (33)
- PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
- Embedded Clusters in Molecular Clouds
- The Dark Energy Survey: more than dark energy - an overview
- The Star Formation History of the Large Magellanic Cloud
- The Star Formation History of the Small Magellanic Cloud
- Clustering of Local Group distances: publication bias or correlated measurements? I. The Large Magellanic Cloud
- A general catalogue of extended objects in the Magellanic System
- Ages and Luminosities of Young SMC/LMC Star Clusters and the recent Star Formation History of the Clouds
- A Search for Old Star Clusters in the Large Magellanic Cloud
- SMASH - Survey of the MAgellanic Stellar History
- ASteCA - Automated Stellar Cluster Analysis
- Comparing the Ancient Star Formation Histories of the Magellanic Clouds
- The VMC Survey IV. The LMC star formation history and disk geometry from four VMC tiles
- The age-metallicity relationship of the Large Magellanic Cloud field star population from wide-field Washington photometry
- New Photometry for the Intermediate-age LMC Globular Cluster NGC 2121 and the Nature of the LMC Age Gap
- Mean age gradient and asymmetry in the star formation history of the Small Magellanic Cloud
- Washington photometry of candidate star clusters in the Small Magellanic Cloud
- The Astro-WISE Optical Image Pipeline: Development and Implementation
- The VMC survey -- XLIII. The spatially resolved star formation history across the Large Magellanic Cloud
- Photometry of Magellanic Cloud clusters with the Advanced Camera for Surveys - II. The unique LMC cluster ESO 121-SC03
- STEP: The VST survey of the SMC and the Magellanic Bridge. I. Overview and first results
- Dynamical masses and mass-to-light ratios of resolved massive star clusters -- II. Results for 26 star clusters in the Magellanic Clouds
- Star Clusters in the Magellanic Clouds-1: Parameterisation and Classification of 1072 Clusters in the LMC
- Physical properties of star clusters in the outer LMC as observed by the Dark Energy Survey
- Star cluster formation history along the minor axis of the Large Magellanic Cloud
- The VMC Survey - XII. Star cluster candidates in the Large Magellanic Cloud
- The VMC survey - XVI. Spatial variation of the cluster-formation activity in the innermost regions of the Large Magellanic Cloud
- A search for star clusters in the outskirts of the Large Magellanic Cloud: indication of clusters in the age gap
- The star formation history of the Large Magellanic Cloud as seen by star clusters and stars
- A catalogue of Large Magellanic Cloud star clusters observed in the Washington photometric system
- A genuine Large Magellanic Cloud age gap star cluster
- Revisiting newly Large Magellanic Cloud age gap star clusters
- Astrophysical properties of newly discovered Magellanic Cloud star clusters