The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies ...

• Main Authors: Santucci, Giulia, Brough, Sarah, van de Sande, Jesse, McDermid, Richard, Barsanti, Stefania, Bland-Hawthorn, Joss, Bryant, Julia J., Croom, Scott M., Lagos, Claudia, Lawrence, Jon S., Owers, Matt S., van de Ven, Glenn, Vaughan, Sam P., Yi, Sukyoung K.
• Format: Text
• Language: unknown
• Published: arXiv 2023
• Subjects: Astrophysics of Galaxies astro-ph.GA; FOS Physical sciences; sami
• Online Access: https://dx.doi.org/10.48550/arxiv.2303.04161; https://arxiv.org/abs/2303.04161

Most dynamical models of galaxies to date assume axisymmetry, which is not representative of a significant fraction of massive galaxies. We have built triaxial orbit-superposition Schwarzschild models of galaxies observed by the SAMI Galaxy Survey, in order to reconstruct their inner orbital structure and mass distribution. The sample consists of 153 passive galaxies with total stellar masses in the range $10^{9.5}$ to $10^{12} M_{\odot}$. We present an analysis of the internal structures and intrinsic properties of these galaxies as a function of their environment. We measure their environment using three proxies: central or satellite designation, halo mass and local $5^{th}$ nearest neighbour galaxy density. We find that although these intrinsic properties correlate most strongly with stellar mass, environment does play a secondary role: at fixed stellar mass, galaxies in the densest regions are more radially anisotropic. In addition, central galaxies, and galaxies in high local densities show lower values ... : 21 pages. Accepted for publication in MNRAS ...