The physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies

The physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies

The stellar surface density within the inner 1 kpc (ς1) has become a popular tool for understanding the growth of galaxies and its connection with the quenching of star formation. The emerging picture suggests that building a central dense core is a necessary condition for quenching. However, it is...

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Bibliographic Details
Main Authors: Bland-Hawthorn, J. (Author), Brough, S. (Author), Bryant, J.J (Author), Catinella, B. (Author), Cortese, L. (Author), Croom, S. (Author), Fraser-Mckelvie, A. (Author), Harborne, K.E (Author), Sweet, S. (Author), Van De Sande, J. (Author), Woo, J. (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
Subjects:
Dispersions
Galaxies
galaxies: bulges
galaxies: disc
galaxies: evolution
galaxies: kinematics and dynamics
Galaxies: Kinematics and dynamics
galaxies: photometry
Galaxies: photometry
Galaxy evolution
Galaxy: disks
Galaxy:bulge
Kinematics
Physical connections
Quenching
Spin dynamics
Stars
Stellar kinematics
Stellar surfaces
Stellars
Surface density
Surveys
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