A dynamical model for the spiral galaxy ngc 3359
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| Format: | Artículo científico |
| Sprache: | en |
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Universidad Nacional Autónoma de México
2008
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| _version_ | 1876463627933843456 |
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| author | M. Rozas |
| author_facet | M. Rozas |
| contents | A dynamical model for the spiral galaxy ngc 3359 M. Rozas Física, Astronomía y Matemáticas galaxies: individual (NGC 3359) galaxies: kinematics and dynamics galaxies: spiral In this work we have determined a dynamical model for NGC 3359. This isa strongly barred spiral galaxy with a complex structure, within which we can seean annular zone of intense star formation. In this work we present self consistentnumerical simulations of molecular gas in NGC 3359; and using the potential derivedfrom an I band image, we attempt to find the parameters responsible for thekinematics and morphology of the observed gas. The best results are obtained fora two pattern speed model: the central region (up to 15´´) corresponding to thenuclear bar which rotates with a Ωs=100 km s−1 kpc−1; and the main bar + outerspiral, decoupled from the nuclear region, which rotates with a angular velocity, Ωp= 27 km s−1 kpc−1. The model successfully reproduces the complex structure inHα of the galaxy in the internal 20´´ zone, which cannot really be explained with aunique mode pattern. 2008 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57144105 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.1 Vol.44 |
| format | Artículo científico |
| id | redalyc_57144105 |
| institution | Redalyc |
| language | en |
| publishDate | 2008 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | A dynamical model for the spiral galaxy ngc 3359 M. Rozas Física, Astronomía y Matemáticas galaxies: individual (NGC 3359) galaxies: kinematics and dynamics galaxies: spiral A dynamical model for the spiral galaxy ngc 3359 M. Rozas Física, Astronomía y Matemáticas galaxies: individual (NGC 3359) galaxies: kinematics and dynamics galaxies: spiral In this work we have determined a dynamical model for NGC 3359. This isa strongly barred spiral galaxy with a complex structure, within which we can seean annular zone of intense star formation. In this work we present self consistentnumerical simulations of molecular gas in NGC 3359; and using the potential derivedfrom an I band image, we attempt to find the parameters responsible for thekinematics and morphology of the observed gas. The best results are obtained fora two pattern speed model: the central region (up to 15´´) corresponding to thenuclear bar which rotates with a Ωs=100 km s−1 kpc−1; and the main bar + outerspiral, decoupled from the nuclear region, which rotates with a angular velocity, Ωp= 27 km s−1 kpc−1. The model successfully reproduces the complex structure inHα of the galaxy in the internal 20´´ zone, which cannot really be explained with aunique mode pattern. 2008 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57144105 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.1 Vol.44 |
| title | A dynamical model for the spiral galaxy ngc 3359 |
| topic | Física, Astronomía y Matemáticas galaxies: individual (NGC 3359) galaxies: kinematics and dynamics galaxies: spiral |
| url | https://www.redalyc.org/articulo.oa?id=57144105 |