activity
20202026
most citedDoes NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster?

37 citations · 170 across the 17 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2026

Central stellar depletion in the Draco dwarf from Subaru photometry

Eduardo Vitral, Kyosuke S. Sato, Jorge Peñarrubia +2

Dark matter subhaloes are a fundamental prediction of the standard cosmological model, but their low-mass population remains difficult to constrain observationally. Recent work has…

astro-ph.GA2026

Dynamical friction vs. subhalo heating in Cold Dark Matter haloes

Jorge Peñarrubia, Pierfrancesco Di Cintio, Eduardo Vitral +1

The orbital evolution of massive stellar systems embedded in dark matter haloes is governed by competing processes. Dynamical friction removes orbital energy, whereas fluctuations…

astro-ph.GA2026

Neighbors, Not Kin: Kinematic evidence for tidal tails from NGC 7492 along the Sagittarius stream

Camila Navarrete, Álvaro Rojas-Arriagada, Andrés E. Piatti +8

The formation, extension, and morphology of extra-tidal stars around globular clusters depend on the internal kinematics of the host cluster and the Galactic potential. Tracing the…

astro-ph.GA2026

Structural Diversity Among the Milky Way's Dwarf Spheroidal Satellites

Matthew G. Walker, Raphaël Errani, Andrew B. Pace +3

We fit a flexible double power-law (`') model to the stellar density fields observed for the Milky Way's known dwarf spheroidal satellite galaxies. We show that where standard…

astro-ph.GA2026

Reconstructing the orbits of Milky Way dwarf galaxies: A Large Magellanic Cloud perspective

Alberto Manuel Martínez-García, Andrés del Pino, Roeland P. van der Marel +14

The orbital histories of the dwarf satellites of the Milky Way (MW) are key to understanding their evolution and placing their present-day properties in a dynamical context. We pre…

astro-ph.IM2026

Hubble Astrometry for the Local Group and Beyond in the 2030s

S. Tony Sohn, Paul Bennet, Kevin Andrew McKinnon +23

Hubble's long, stable astrometric baseline creates a rare opportunity for discovery in the Local Group and beyond. Many nearby galaxies, streams, and star clusters already have arc…

astro-ph.GA2025

The Proper Motion of Draco II with HST using Multiple Reference Frames and Methodologies

Jack T. Warfield, Kevin A. McKinnon, Sangmo Tony Sohn +13

We present proper motion (PM) measurements for Draco II, an ultra-faint dwarf satellite of the Milky Way. These PMs are measured using two epochs of Hubble Space Telescope Advanced…

astro-ph.GA2025★ 1 cited

Signatures of dark subhalos in dwarf spheroidal galaxies: I. Fluctuations in surface density

Eduardo Vitral, Jorge Peñarrubia, Matthew G. Walker

Dark matter (DM) subhalos offer critical tests of cosmological models through their abundance and properties, yet most remain undetectable due to their lack of stars. We investigat…

astro-ph.GA2025★ 5 cited

HSTPROMO Internal Proper Motion Kinematics of Dwarf Spheroidal Galaxies: II. Velocity Anisotropy and Dark Matter Cusp Slope of Sculptor

Eduardo Vitral, Roeland P. van der Marel, Sangmo Tony Sohn +8

We analyze three epochs of HST imaging over 20 years for the Sculptor dwarf spheroidal galaxy, measuring precise proper motions for 119 stars and combining them with 1760 existing…

astro-ph.GA2025

Gravothermal expansion of dwarf spheroidal galaxies heated by dark subhaloes

Jorge Peñarrubia, Raphaël Errani, Eduardo Vitral +1

We use analytical and -body methods to study the evolution of dwarf spheroidal galaxies (dSphs) embedded in dark matter (DM) haloes that host a sizeable subhalo population. Dark…

astro-ph.GA2024★ 18 cited

HSTPROMO Internal Proper Motion Kinematics of Dwarf Spheroidal Galaxies: I. Velocity Anisotropy and Dark Matter Cusp Slope of Draco

Eduardo Vitral, Roeland P. van der Marel, Sangmo Tony Sohn +8

We analyze four epochs of HST imaging over 18 years for the Draco dwarf spheroidal galaxy. We measure precise proper motions (PMs) for hundreds of stars and combine these with exis…

astro-ph.GA2023

BP3M: Bayesian Positions, Parallaxes, and Proper Motions derived from the Hubble Space Telescope and Gaia data

Kevin A. McKinnon, Andrés del Pino, Constance M. Rockosi +9

We present a hierarchical Bayesian pipeline, BP3M, that measures positions, parallaxes, and proper motions (PMs) for cross-matched sources between Hubble~Space~Telescope (HST) imag…

astro-ph.GA2023★ 18 cited

An elusive dark central mass in the globular cluster M4

Eduardo Vitral, Mattia Libralato, Kyle Kremer +4

Recent studies of nearby globular clusters have discovered excess dark mass in their cores, apparently in an extended distribution, and simulations indicate that this mass is compo…

astro-ph.GA2022★ 31 cited

Stellar graveyards: Clustering of compact objects in globular clusters NGC 3201 and NGC 6397

Eduardo Vitral, Kyle Kremer, Mattia Libralato +2

We analyse Gaia EDR3 and re-calibrated HST proper motion data from the core-collapsed and non core-collapsed globular clusters NGC 6397 and NGC 3201, respectively, with the Bayesia…

astro-ph.GA2021★ 12 cited

Properties of globular clusters formed in dark matter mini-halos

Eduardo Vitral, Pierre Boldrini

We seek to differentiate dynamical and morphological attributes between globular clusters (GCs) that were formed inside their own dark matter (DM) mini-halo, and those who were not…

astro-ph.GA2021★ 10 cited

Absence of obvious tidal tails around the globular cluster NGC 6397

Pierre Boldrini, Eduardo Vitral

In this work, we use body simulations performed on GPU to trace the past 10 Gyr dynamical history of a globular cluster (GC) similar to NGC~6397 in the tidal field of a Milky W…

astro-ph.GA2021★ 20 cited

BALRoGO: Bayesian Astrometric Likelihood Recovery of Galactic Objects -- Global properties of over one hundred globular clusters with Gaia EDR3

Eduardo Vitral

We present BALRoGO: Bayesian Astrometric Likelihood Recovery of Galactic Objects, a public code to measure the centers, effective radii, and bulk proper motions of Milky Way globul…

astro-ph.GA2020★ 37 cited

Does NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster?

Eduardo Vitral, Gary A. Mamon

We analyze proper motions from the Hubble Space Telescope (HST) and the second Gaia data release along with line-of-sight velocities from the MUSE spectrograph to detect imprints o…

astro-ph.GA2020★ 18 cited

A Precise Analytical Approximation for the Deprojection of the Sérsic Profile

Eduardo Vitral, Gary A. Mamon

The Sérsic model is known to fit well the surface brightness (or surface density) profiles of elliptical galaxies and galaxy bulges, and possibly for dwarf spheroidal galaxies and…