The PARSEC view of star formation in galaxy centres: from protoclusters to star clusters in an early-type spiral
Understanding star formation in galaxies requires resolving the physical scale on which star formation often occurs: the scale of star clusters. We present a multiwavelength, eight-parsec resolution study of star formation in the circumnuclear star cluster and molecular gas rings of the early-type spiral NGC 1386. The cluster ring formed
Prieto, Almudena et al.
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2024