演講資訊

摘要：

The galaxy integrated star formation rate(SFR)-stellar mass(M*) relation holds important information for understanding the star formation history and evolution of galaxies. Although the SFR-M* relation has been reported with a variety of different data sets, their appearance can vary significantly from one to another. In this work, we determine what controls the integrated and the spatially-resolved SFR-M* relation in both star-forming and quiescent galaxies by linking the spatially resolved SFR-M* relation with various galaxy properties such as stellar mass and bulge-to-total light ratio using MaNGA data (Mapping Nearby Galaxies at APO).