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MAGNUS II: Rotational support of massive early-type galaxies decreased over the past 7 billion years

Mozumdar, Pritom et al.
arXiv (All) · Papers
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astrophysics-of-galaxies
Understanding how the internal kinematics of massive galaxies evolve is key to constraining the physical processes that drive their assembly. We investigate the evolution of rotational support in massive ($\log M_{\ast}/M_{\odot} \geq 10.6$) early-type galaxies (ETGs) over the past $\sim$7 Gyr. We u
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