THE IMPRINT of RADIAL MIGRATION on the VERTICAL STRUCTURE of GALAXY DISKS

We use numerical simulations to examine the effects of radial migration on the vertical structure of galaxy disks. The simulations follow three exponential disks of different mass but similar circular velocity, radial scalelength, and (constant) scale height. The disks develop different non-axisymme...

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Autores:
Tipo de recurso:
Fecha de publicación:
2016
Institución:
Universidad de Medellín
Repositorio:
Repositorio UDEM
Idioma:
eng
OAI Identifier:
oai:repository.udem.edu.co:11407/3155
Acceso en línea:
http://hdl.handle.net/11407/3155
Palabra clave:
galaxies: kinematics and dynamics
Galaxy: disk
Galaxy: evolution
stars: kinematics and dynamics
Rights
restrictedAccess
License
http://purl.org/coar/access_right/c_16ec