Young star-forming clumps in four spiral galaxies show fractal clustering only below a galaxy-dependent scale of 0.5 to 3.1 kpc, with the hierarchy dissipating within 10 to 50 Myr.
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Tracing Hierarchical Star Formation out to Kiloparsec Scales in Nearby Spiral Galaxies with UVIT
Young star-forming clumps in four spiral galaxies show fractal clustering only below a galaxy-dependent scale of 0.5 to 3.1 kpc, with the hierarchy dissipating within 10 to 50 Myr.