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20242026
most citedPrecise Measurements of the LMC Bar's Geometry With Gaia DR3 and a Novel Solution to Crowding Induced Incompleteness in Star Counting

12 citations · 24 across the 5 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

The Role of Dark Matter in Driving Disk Perturbations: Application to LMC-SMC Like Galaxy Interactions

Himansh Rathore, Hayden R. Foote, Gurtina Besla +6

Dark-matter (DM) models predict that satellite galaxies distort their host's DM halo. As such, both the satellite and the distorted halo can perturb the host's stellar disk. The LM…

astro-ph.GA2026

A Statistical Framework to Identify Kinematically Outlying LMC Globular Clusters and Implications for the LMC's Dark Matter Profile

Tamojeet Roychowdhury, Navdha, Himansh Rathore +1

The LMC's Globular Clusters (GCs) bring a novel opportunity to understand the LMC's assembly history and dark matter (DM) properties, provided the kinematically outlying GCs can be…

astro-ph.GA2026★ 1 cited

Mapping the Distorted Dark Matter Distribution of the LMC-SMC System Prior to Milky Way Infall with Basis Function Expansions

Hayden R. Foote, Himansh Rathore, Gurtina Besla +6

The SMC orbits within the LMC's dark matter (DM) halo in a 1:10 mass-ratio encounter. The LMC:Milky Way (MW) interaction is also 1:10, and is expected to perturb the MW…

astro-ph.GA2025★ 4 cited

A Galactic Transformation -- Understanding the SMC's Structural and Kinematic Disequilibrium

Himansh Rathore, Gurtina Besla, Roeland P. van der Marel +1

The SMC is in disequilibrium. Gas line-of-sight (LoS) velocity maps show a gradient of km s, generally interpreted as a rotating gas disk consistent with the Tully-…

astro-ph.GA2025★ 7 cited

Response of the LMC's Bar to a Recent SMC Collision and Implications for the SMC's Dark Matter Profile

Himansh Rathore, Gurtina Besla, Kathryne J. Daniel +1

The LMC's stellar bar is offset from the outer disk center, tilted from the disk plane, and does not drive gas inflows. These properties are atypical of bars in gas-rich galaxies,…

astro-ph.GA2024★ 12 cited

Precise Measurements of the LMC Bar's Geometry With Gaia DR3 and a Novel Solution to Crowding Induced Incompleteness in Star Counting

Himansh Rathore, Yumi Choi, Knut A. G. Olsen +1

We present new measurements of the two-dimensional (2-D) geometry of the LMC's stellar bar with precise astrometric observations of red clump stars in Gaia DR3. We develop a novel…