KMHK 1762: Another star cluster in the Large Magellanic Cloud age gap
KMHK 1762: Another star cluster in the Large Magellanic Cloud age gap
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Author / Creator
Gatto, M , Ripepi, V , Bellazzini, M , Tosi, M , Tortora, C , Cignoni, M , Dall'Ora, M , Cioni, M -R L , Cusano, F , Longo, G , Marconi, M , Musella, I , Schipani, P and Spavone, M
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
The star cluster (SC) age distribution of the Large Magellanic Cloud (LMC) exhibits a gap from \(\sim\) 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 wher...
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Full title
KMHK 1762: Another star cluster in the Large Magellanic Cloud age gap
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TN_cdi_proquest_journals_2692480279
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2692480279
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.2207.09478
