The Fraction of Clumpy Galaxies in JADES over $2
Abstract: High-redshift galaxies exhibit compact regions of intense star formation, known as “clumps,” which are conspicuous in the rest-frame ultraviolet. Studying them can shed light on how they form and evolve and inform theoretical models of galaxy evolution. We examine the evolution of clumpy galaxies with redshift and stellar mass over ${2
2026-04-08
Comments are closed, but trackbacks and pingbacks are open.