most citedThe dark matter profile of the Milky Way inferred from its circular velocity curve

13 citations · 22 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20248 cited

Confronting the Diversity Problem: The Limits of Galaxy Rotation Curves as a tool to Understand Dark Matter Profiles

Isabel S. Sands, Philip F. Hopkins, Xuejian Shen +9

While galaxy rotation curves provide one of the most powerful methods for measuring dark matter profiles in the inner regions of rotation-supported galaxies, at the dwarf scale the…

astro-ph.GA2024

The Rise of the -Process in the Gaia-Sausage/Enceladus Dwarf Galaxy

Xiaowei Ou, Alexander P. Ji, Anna Frebel +2

Neutron star mergers (NSMs) produce copious amounts of heavy r-process elements after a time delayed inspiral process. Once NSMs are present in a galaxy, r-process elements, such a…

astro-ph.GA2024

Signatures of tidal disruption of the Hercules ultra-faint dwarf galaxy

Xiaowei Ou, Anirudh Chiti, Nora Shipp +6

The Hercules ultra-faint dwarf galaxy (UFD) has long been hypothesized to be tidally disrupting, yet no conclusive evidence has been found for tidal disruption owing partly to diff…

astro-ph.GA20231 cited

Synthetic Gaia DR3 surveys from the FIRE cosmological simulations of Milky-Way-mass galaxies

Tri Nguyen, Xiaowei Ou, Nondh Panithanpaisal +4

The third data release (DR3) of Gaia has provided a five-fold increase in the number of radial velocity measurements of stars, as well as a stark improvement in parallax and proper…

astro-ph.GA202313 cited

The dark matter profile of the Milky Way inferred from its circular velocity curve

Xiaowei Ou, Anna-Christina Eilers, Lina Necib +1

In this paper, we construct the circular velocity curve of the Milky Way out to kpc, providing an updated model of the dark matter density profile. We derive precise para…