The properties of inside-out assembled galaxies at z < 0.1

• DOI: 10.1017/s1743921320003348
• Publication Date: 2021-01-29T09:48:31Z
• Authors: Dejene Zewdie; Mirjana Pović; Manuel Aravena; Roberto J. Assef; Asrate Gaulle
• Keywords: Stellar mass; Star (game theory)

Abstract In this work, we study the properties of galaxies that are showing inside-out assembly (which call assembled galaxies; IOAGs), with main aim to understand better their and morphological transformation. We analysed a sample from Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8), stellar masses in range log M * = 10.73 – 11.03 ⊙ at z &lt; 0.1, analyze location mass-SFR color-stellar mass diagram. found IOAGs have different spectroscopic properties, most them being classified either as AGN or composite. majority our sources located below sequence star formation SFR-stellar diagram, green valley red argue seem correspond transition area where moving star-forming quiescent, blue cloud and/or recently quenched galaxies.