Starburst galaxies in the COSMOS field: clumpy star-formation at redshift 0 < z < 0.5
Context. At high redshift, starburst galaxies present irregular morphologies with 10-20% of their star formation occurring in giant clumps. These clumpy galaxies are considered the progenitors of local disk galaxies. To understand the properties of starbursts at intermediate and low redshift, it is fundamental to track their evolution and the
Hinojosa-Goñi, R. et al.
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2016