Evolution of spatially resolved star formation main sequence and surface density profiles in massive disc galaxies at 0 ≲ z ≲ 1: inside–out stellar mass buildup and quenching

Authors :: Abdurro'uf
Masayuki Akiyama
Source :: Monthly Notices of the Royal Astronomical Society. 479:5083-5100
Publication Year :: 2018
Publisher :: Oxford University Press (OUP), 2018.
Abstract: We investigate a relation between surface densities of star formation rate (SFR) and stellar mass ($M_{*}$) at a $\sim 1$ kpc scale namely spatially resolved star formation main sequence (SFMS) in massive ($\log(M_{*}/M_{\odot})>10.5$) face-on disc galaxies at $0.01<br />Comment: 20 pages, 21 figures. Updated with some supporting appendixes. Accepted by MNRAS

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