ON THE FORMATION OF THE DISK OF SATELLITES OF THE MILKY WAY: SIMULATION OF THE COLLISION OF TWO GALAXIES

At present there is some evidence showing that the satellite galaxies of the Milky Way might be distributed on a disc structure, known as the disc of satellites. In this paper a study on the possible formation of the disc of satellites of the Milky Way as the result of a collision between two disc g...

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Main Authors: Diana J. Cubillos Jara, Rigoberto A. Casas Miranda
Format: Article
Language:English
Published: Universidad Nacional de Colombia 2014-01-01
Series:Momento
Subjects:
Online Access:https://revistas.unal.edu.co/index.php/momento/article/view/48027
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author Diana J. Cubillos Jara
Rigoberto A. Casas Miranda
author_facet Diana J. Cubillos Jara
Rigoberto A. Casas Miranda
author_sort Diana J. Cubillos Jara
collection DOAJ
description At present there is some evidence showing that the satellite galaxies of the Milky Way might be distributed on a disc structure, known as the disc of satellites. In this paper a study on the possible formation of the disc of satellites of the Milky Way as the result of a collision between two disc galaxies ~10 Gyr ago is shown. The study is carried out by numerical N-Body simulations with 10^6 particles in each galaxy and with a mass ratio of 4 to 1, being the larger galaxy similar to the Milky Way. The results show how tidal forces between the two colliding galaxies produce a spatial distribution of debris, where possible groups of stars lie nearly perpendicular to the plane of the host galaxy, showing similarity in this feature with the disc of satellites of the Milky Way.
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spelling doaj.art-9c85548c8560430899ca06338ebf19012022-12-22T01:57:27ZengUniversidad Nacional de ColombiaMomento0121-44702500-80132014-01-0104811738673ON THE FORMATION OF THE DISK OF SATELLITES OF THE MILKY WAY: SIMULATION OF THE COLLISION OF TWO GALAXIESDiana J. Cubillos Jara0Rigoberto A. Casas Miranda1Universidad Nacional de Colombia, Bogotá.Universidad Nacional de Colombia, Bogotá.At present there is some evidence showing that the satellite galaxies of the Milky Way might be distributed on a disc structure, known as the disc of satellites. In this paper a study on the possible formation of the disc of satellites of the Milky Way as the result of a collision between two disc galaxies ~10 Gyr ago is shown. The study is carried out by numerical N-Body simulations with 10^6 particles in each galaxy and with a mass ratio of 4 to 1, being the larger galaxy similar to the Milky Way. The results show how tidal forces between the two colliding galaxies produce a spatial distribution of debris, where possible groups of stars lie nearly perpendicular to the plane of the host galaxy, showing similarity in this feature with the disc of satellites of the Milky Way.https://revistas.unal.edu.co/index.php/momento/article/view/48027Grupo LocalVía Láctea: Disco de Satélitesgalaxias.
spellingShingle Diana J. Cubillos Jara
Rigoberto A. Casas Miranda
ON THE FORMATION OF THE DISK OF SATELLITES OF THE MILKY WAY: SIMULATION OF THE COLLISION OF TWO GALAXIES
Momento
Grupo Local
Vía Láctea: Disco de Satélites
galaxias.
title ON THE FORMATION OF THE DISK OF SATELLITES OF THE MILKY WAY: SIMULATION OF THE COLLISION OF TWO GALAXIES
title_full ON THE FORMATION OF THE DISK OF SATELLITES OF THE MILKY WAY: SIMULATION OF THE COLLISION OF TWO GALAXIES
title_fullStr ON THE FORMATION OF THE DISK OF SATELLITES OF THE MILKY WAY: SIMULATION OF THE COLLISION OF TWO GALAXIES
title_full_unstemmed ON THE FORMATION OF THE DISK OF SATELLITES OF THE MILKY WAY: SIMULATION OF THE COLLISION OF TWO GALAXIES
title_short ON THE FORMATION OF THE DISK OF SATELLITES OF THE MILKY WAY: SIMULATION OF THE COLLISION OF TWO GALAXIES
title_sort on the formation of the disk of satellites of the milky way simulation of the collision of two galaxies
topic Grupo Local
Vía Láctea: Disco de Satélites
galaxias.
url https://revistas.unal.edu.co/index.php/momento/article/view/48027
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