Influence of Dark Matter Subhalos on the Formation of the Galaxy Spiral Arms

The dynamical stability of disk galaxies in a ΛCDM cosmology is a fundamental topic in galactic evolution, particularly in the presence of perturbers. In this study, we analyze the structural and kinematic properties of a simulated galactic disk, focusing on the effects of satellite interactions on...

Full description

Autores:

López Aristizábal, Ana María

Tipo de recurso:

Trabajo de grado de pregrado

Fecha de publicación:

2025

Institución:

Universidad de Antioquia

Repositorio:

Repositorio UdeA

Idioma:

eng

OAI Identifier:

oai:bibliotecadigital.udea.edu.co:10495/45946

Acceso en línea:

https://hdl.handle.net/10495/45946

Palabra clave:

Galaxias espirales - Estructura
Spiral galaxies - Structure
Galaxias - Formación
Galaxies - Formation
Materia oscura (Astronomía)
Dark matter (Astronomy)
Halos galácticos
Galactic halos
Problema de los cuerpos múltiples
Many-body problem
Galaxias enanas
Dwarf galaxies
Dinámica galáctica
Galactic dynamics
Hidrodinámica - Modelos matemáticos
Hydrodynamics - Mathematical models
http://id.loc.gov/authorities/subjects/sh2003009307
http://id.loc.gov/authorities/subjects/sh94008658
http://id.loc.gov/authorities/subjects/sh87007317
http://id.loc.gov/authorities/subjects/sh91001801
http://id.loc.gov/authorities/subjects/sh85080793
http://id.loc.gov/authorities/subjects/sh85040180
http://id.loc.gov/authorities/subjects/sh2003009304
http://id.loc.gov/authorities/subjects/sh2008105960

Rights

openAccess

License

http://creativecommons.org/licenses/by-nc-sa/4.0/