Kinematical decomposition of stellar populations in disc galaxies

Bibcode
2015hsa8.conf..154C
Cacho, R.; Seidel, M. K.; Ruiz-Lara, T.; Sánchez-Blázquez, P.; Falcón-Barroso, J.; Pérez, I.; Vogt, F. P. A.; Ness, M.; Freeman, K. C.; Aniyam, S.
Referencia bibliográfica

Highlights of Spanish Astrophysics VIII, Proceedings of the XI Scientific Meeting of the Spanish Astronomical Society held on September 8-12, 2014, in Teruel, Spain, ISBN 978-84-606-8760-3. A. J. Cenarro, F. Figueras, C. Hernández-Monteagudo, J. Trujillo Bueno, and L. Valdivielso (eds.), p. 154-159

Advertised on:
5
2015
Número de autores
10
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
Understanding how different stellar populations evolve in different regions is a key to understand the evolution of galaxies. Traditionally the kinematics and stellar populations in galaxies have been obtained separately and unrelatedly, sometimes ignoring the other one. In this pilot study we simultaneously disentangle the stellar populations (characterizing their age and metallicity) and associate them with the stellar kinematics (velocity and velocity dispersion) in the bulge of three very different disc galaxies using high resolution IFS data.
Tipo
Sin árbitro

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