Imprint of Pressure on Characteristic Dark Matter Profiles: The Case of ESO0140040

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 <i>pseudo-isothermal</i>, <i>exponential sphere</i>, <i>Burkert</i>, <i>Navarro-Frenk-White</i>, <i>Moore</i>...

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Bibliographic Details
Main Authors: Kuantay Boshkayev, Talgar Konysbayev, Ergali Kurmanov, Orlando Luongo, Marco Muccino
Format: Article
Language:English
Published: MDPI AG 2020-10-01
Series:Galaxies
Subjects:
dark matter
rotational curves
equation of state
perturbations
optical properties
Online Access:https://www.mdpi.com/2075-4434/8/4/74

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