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Compared to the simulated galaxy from the IllustrisTNG below, the above simulations clearly show the protruding structure near the main disk, especially in panel 3.
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This repository contains files and code for a IllustrisTNG research project that investigates the effects of varying observing angles on the M_BH-Bulge Velocity Dispersion relation. Code from the MaNGIA's data release (Sarmiento+ 2022) helped the project significantly. Credits to https://github.com/reginasar/TNG_MaNGA_mocks.
ZiyuanYinn/TNG
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This repository contains files and code for a IllustrisTNG research project that investigates the effects of varying observing angles on the M_BH-Bulge Velocity Dispersion relation. Code from the MaNGIA's data release (Sarmiento+ 2022) helped the project significantly. Credits to https://github.com/reginasar/TNG_MaNGA_mocks.
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