The Kinematics of the Local Group in a Cosmological Context
ABSTRACT: Recent observations constrained the tangential velocity of M31 with respect to the Milky Way to be vM31, tan < 34.4 km s−1and the radial velocity to be in the range vM31, rad = −109 ± 4.4 km s−1. In this study we use a large volume high-resolution N-body cosmological simulation (Bolshoi...
- Autores:
-
Bustamante Jaramillo, Sebastián
Forero Romero, J. E.
Hoffman, Y.
Gottlober, S.
Yepes, G.
- Tipo de recurso:
- Article of investigation
- Fecha de publicación:
- 2013
- Institución:
- Universidad de Antioquia
- Repositorio:
- Repositorio UdeA
- Idioma:
- eng
- OAI Identifier:
- oai:bibliotecadigital.udea.edu.co:10495/34945
- Acceso en línea:
- https://hdl.handle.net/10495/34945
- Palabra clave:
- Vía Lactea
Milky way
Cinemática
Kinematics
Dinámica
Dynamics
- Rights
- openAccess
- License
- http://creativecommons.org/licenses/by/2.5/co/