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What is Stellar Mass Buildup in Disk Galaxies about?

This document discusses spatially resolved stellar mass buildup and quenching in massive disk galaxies over the last 10 billion years using spatially resolved SED fitting. The study finds that massive disk galaxies tend to build up their stellar mass and quench star formation progressively from the central region to the outskirts, indicating an inside-out pattern of stellar mass buildup and quenching. Spatially resolved star formation rates are found to correlate with stellar mass surface densities in both

Author

Alberto Ramirez

Language

EN