Dynamical Hotness, Star Formation Quenching, and Growth of Supermassive Black Holes

A stellar system is dynamically hot when its kinetic energy is dominated by random motion represented by the velocity dispersion σ _hot . We use MaNGA data to obtain the inner and outer dispersion of a galaxy, σ _in and σ _out , to characterize its dynamical status and study its connection with star...

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Hlavní autoři:	Hui Hong, Huiyuan Wang, H. J. Mo, Ziwen Zhang, Guangwen Chen, Wentao Luo, Tinggui Wang, Pengfei Li, Renjie Li, Yao Yao, Aoxiang Jiang
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2023-01-01
Edice:	The Astrophysical Journal
Témata:	Galaxy formation Galaxy evolution Galaxy classification systems Galaxy quenching Galaxy dynamics Active galactic nuclei
On-line přístup:	https://doi.org/10.3847/1538-4357/ace96f
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