The Timescales of Star Cluster Emergence: The Case of NGC 4449

The Astrophysical Journal(2024)

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Abstract
We survey the young star cluster population in the dwarf galaxy NGC4449 with the goal of investigating how stellar feedback may depend on the clusters' properties. Using Ultraviolet(UV)-optical-NearIR(NIR) photometry obtained from the Hubble Space Telescope, we have recovered 99 compact sources exhibiting emission in the Paβ hydrogen recombination line. Our analysis reveals these sources possess masses 10^2More
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Key words
Interstellar dust,Young star clusters,Dwarf galaxies,Interstellar dust extinction
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