Modell zur Entstehung eines Rings aus Dunkler Materie in der Milchstra{\ss}enebene
Rapha\"el Errani (Athenaeum Stade, Germany)

TL;DR
This paper models the formation of a dark matter ring in the Milky Way's plane at 14 kiloparsecs, explaining its origin through dwarf galaxy accretion using a semi-analytical approach.
Contribution
It introduces a semi-analytical model demonstrating how dwarf galaxy infall can form a dark matter ring in the Milky Way, with specific orbital constraints and mass limits.
Findings
Ring formation explained by single or multiple dwarf galaxy infalls
Orbital eccentricity must be ≤ 0.2 for formation
Mass limits for dwarf galaxies involved in ring formation
Abstract
Both the distribution of hydrogen and the rotation curve of the Milky Way indicate the existence of a ring of Cold Dark Matter in the galactic plane with a radius of 14 kiloparsecs around the galactic centre. Using a semianalytical model, the formation of such a structure by the accretion of dwarf galaxies is simulated. The formation of the ring can be explained by the infall of a single dwarf galaxy, as well as by the infall of several dwarf galaxies under the condition that the eccentricity of the orbits is not larger than 0.2 and the inclination of the orbits is small. Also exclusion limits for the mass of dwarf galaxies, which contributed to the formation of the ring, are determined. ----- Die Verteilung von Wasserstoffgas sowie die Rotationskurve der Milchstra{\ss}e deuten auf die Existenz eines Rings aus kalter Dunkler Materie innerhalb der Milchstra{\ss}enebene in einem…
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Taxonomy
TopicsRadio Astronomy Observations and Technology
