The Timescales of Star Cluster Emergence: The Case of NGC 4449
The Astrophysical Journal(2024)
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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