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A boxy bulge in the Milky Way. Inversion of the stellar statistics equation with 2MASS data

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arxiv astro-ph/0504608 v1 pith:66VXOAB2 submitted 2005-04-27 astro-ph

M. Lopez-Corredoira , A. Cabrera-Lavers , O. E. Gerhard This is my paper · ORCID
classification astro-ph
keywords bulgeboxyequationmassstatisticsstellarangleaxial
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abstract

Inverting the stellar statistics equation from 2MASS star counts, we obtain the 3D density distribution of the Galactic bulge as well as its luminosity function in the K-band. This results in a boxy bulge with axial ratios 1:0.5:0.4 and a major axis angle with respect to the Sun-galactic center of $20^\circ-35^\circ $.

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Cited by 1 Pith paper

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  1. Diversity of Fuzzy Dark Matter Solitons

    hep-ph 2024-11 conditional novelty 6.0 of 10

    Environmental effects, especially a central black hole and baryonic matter, can substantially alter fuzzy dark matter soliton profiles, while the soliton's own gravitomagnetic field is negligible.

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