activity
19952026
most citedOrbital Parameters of Merging Dark Matter Halos

248 citations · 2.4k across the 54 of their papers we have counts for

collaborators

54 papers

astro-ph.GA2026

Interacting stellar winds feeding Sgr A*: from the system of mass-losing stars to the binary IRS 16SW

Diego Calderón, Jorge Cuadra, Christopher M. P. Russell +3

The discovery of cold structures around Sgr A* has challenged our understanding of the gas dynamics and thermodynamic state of the plasma in its vicinity. This work aims to constra…

astro-ph.GA2026

Superdiffusion at the Galactic Centre

Pau Amaro Seoane, Kostas Tzanavaris, Reinhard Genzel +14

Tracking S-star cluster orbits around Sgr A* calibrates orbital transport models for space-borne gravitational wave detectors. Standard kinetic theories model this cluster via loca…

astro-ph.GA2026

Stellar rotation of S301 as a macroscopic gyroscope to test general relativity

Pau Amaro Seoane, Xian Chen, Alejandro Torres-Orjuela +16

Stellar trajectories around the Galactic Center provide a testing environment for general relativity. The intrinsic rotation of these stars evolves under covariant transport in cur…

astro-ph.GA2026

S301 and friends: Measuring the spin of Sgr A*

T. Piran, P. Amaro-Seoane, B. Aytac +15

The discovery of S301 (GRAVITY Collaboration et al., 2026) with pericenter distance rp= 280rg and eccentricity e=0.9825, opens the prospect of measuring the spin parameter of Sgr A…

astro-ph.GA2026

Bonnor-Ebert sphere collapse in filamentary structures

Stefan Heigl, Andreas Burkert

Star formation within filaments may arise due to the growth of cores according to linear perturbation theory. This implies a minimum core separation, as shorter modes would not be…

astro-ph.GA2024★ 4 cited

The Milky Way satellite galaxy Leo T: A perturbed cored dwarf

Matias Blaña, Andreas Burkert, Michael Fellhauer +3

The impact of the dynamical state of gas-rich satellite galaxies at the early moments of their infall into their host systems and the relation to their quenching process are not co…