Imprint of Pressure on Characteristic Dark Matter Profiles: The Case of ESO0140040
We investigate the dark matter distribution in the spiral galaxy ESO0140040, employing the most widely used density profiles: the pseudo-isothermal, exponential sphere, Burkert, Navarro-Frenk-White, Moore and Einasto profiles.We infer the model parameters and estimate the total dark matter content from the rotation curve data.For simplicity, we ass