Pith. sign in

REVIEW 1 cited by

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

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

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
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
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 $.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  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.

Pith tools