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astro-ph.GA2024★ 4 cited
Shapes of dark matter haloes with discrete globular cluster dynamics: The example of NGC 5128 (Centaurus A)
Tadeja Veršič, Marina Rejkuba, Magda Arnaboldi +7
Within the CDM cosmology, dark matter haloes are expected to deviate from spherical symmetry. Constraining the halo shapes at large galactocentric distances is challenging due t…
astro-ph.GA2024★ 1 cited
The Mass of the Large Magellanic Cloud from the Three-Dimensional Kinematics of its Globular Clusters
Laura L. Watkins, Roeland P. van der Marel, Paul Bennet
We estimate the mass of the Large Magellanic Cloud (LMC) using the kinematics of 30 LMC globular clusters (GCs). We combine proper motions (PMs) measured with HST, Gaia, or a combi…