196. The rotation curve of our Galaxy

The rotation curve of our Galaxy provides strong constraints on the mass distribution of its major structural components. New Gaia results suggest a strongly revised dependency within the solar circle, and a steepening Keplerian decline beyond 20 kpc, which may indicate the limits of our Galaxy's dark matter halo.

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2024-09-30
DOI
https://doi.org/10.5281/zenodo.14599491
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
0.00
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article

196. The rotation curve of our Galaxy

Zenodo (CERN European Organization for Nuclear Research)
Astronomy and Astrophysical Research
article

196. The rotation curve of our Galaxy

article en

Abstract

The rotation curve of our Galaxy provides strong constraints on the mass distribution of its major structural components. New Gaia results suggest a strongly revised dependency within the solar circle, and a steepening Keplerian decline beyond 20 kpc, which may indicate the limits of our Galaxy's dark matter halo.

Zenodo (CERN European Organization for Nuclear Research)
Openalex Percentile: Top 67%
Astronomy and Astrophysical Research
DOIOpen Access PDFOpenAlex
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196. The rotation curve of our Galaxy · Zenodo (CERN European Organization for Nuclear Research) (2024) | TGRS Research Map | TGRS