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STELLAR ORBITAL STUDIES IN NORMAL SPIRAL GALAXIES: EFFECT OF SPIRAL ARMS ON DISK DYNAMICS

We have built a family of non-axisymmetric potential models for normal non-ba rred spiral galaxies. For this purpose, a three-dimensional self-gravitating model of spiral arms (PERLAS) is used. We analyze the stellar dynamics on the disk plane, varying structural and dynamical parameters such as pit...

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Publié dans:Revista Mexicana de Astronomía y Astrofísica
Auteurs principaux: A. Pérez-Villegas, B. Pichardo, E. Moreno
Format: Artigo
Langue:Inglês
Publié: Universidad Nacional Autónoma de México 2015
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Accès en ligne:https://www.redalyc.org/articulo.oa?id=57150514016
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