Shape Asymmetries and the Relation between Lopsidedness and Radial Alignment in Simulated Galaxies

Shape Asymmetries and the Relation between Lopsidedness and Radial Alignment in Simulated Galaxies

Galaxies are observed to be lopsided, meaning that they are more massive and more extended along one side than the opposite side. In this work, we provide a statistical analysis of the lopsided morphology of 1780 isolated satellite galaxies generated by the TNG50-1 simulation, incorporating the effe...

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Bibliographic Details
Main Authors:	Jinzhi Shen, Xufen Wu, Yirui Zheng, Beibei Guo
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Series:	The Astrophysical Journal
Subjects:	Galaxy dynamics Galaxy dark matter halos Galaxy mass distribution Astronomical simulations
Online Access:	https://doi.org/10.3847/1538-4357/ad07d8

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