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• W2897066435 abstract "Local galaxies from the Sloan Digital Sky Survey are used to provide additional support for an evolutionary pathway in which AGN activity is associated with star-formation quenching. Composite, Seyfert 2 and LINER galaxies account for $sim$60% of all star-formation in massive galaxies ($M_star > 10^{10.5} M_odot$). Inclusion of these galaxies results in a turnover in the $SFR - M_star$ relation for massive galaxies. Our analysis shows that bulge growth has already occurred in the most massive galaxies ($M_star > 10^{10.5}$ $M_odot$), and bulges continue to grow as galaxies quench and redden, $(g-r)$ = 0.5 $rightarrow$ 0.75. Significant bulge growth is also occurring in low mass starburst galaxies ($M_star < 10^{10.5} M_odot$) at 0.5 dex above the main sequence (MS), where we find an increase in $B/T$ from 0.1 $rightarrow$ 0.3 and bluer colours, $(g-r) < 0.25$ compared to low-mass galaxies on the MS." @default.
• W2897066435 created "2018-10-26" @default.
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• W2897066435 date "2018-10-24" @default.
• W2897066435 modified "2023-10-17" @default.
• W2897066435 title "Dissecting the main sequence: AGN activity and bulge growth in the local Universe" @default.
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• W2897066435 doi "https://doi.org/10.1093/mnrasl/sly202" @default.
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