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arXiv · 0810.5300

Modell zur Entstehung eines Rings aus Dunkler Materie in der Milchstraßenebene

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 Milchstraße deuten auf die Existenz eines Rings aus kalter Dunkler Materie innerhalb der Milchstraßenebene in einem Abstand von rund 14 Kiloparsec um das galaktische Zentrum. Es wird mit Hilfe eines semianalytischen Modells die Entstehung eines solchen Rings durch den Einfall von Zwerggalaxien in die Milchstraße simuliert. Die Entstehung des Rings kann sowohl durch einen Einzeleinfall als auch durch den Einfall mehrerer Zwerggalaxien erklärt werden, solange die numerische Exzentrizität der Orbits nicht 0.2 übersteigt und die Inklination der Orbits klein ist. Auch ein die Mindestmasse einer an der Ringentstehung beteiligten Zwerggalaxie beschreibender Zusammenhang ist ermittelt worden.

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BibTeXRIS

Raphaël Errani. 2010-01-15. Modell zur Entstehung eines Rings aus Dunkler Materie in der Milchstraßenebene. https://arxiv.org/abs/0810.5300

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