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20002026
most citedThe Bright Gamma-Ray Burst 991208 - Tight Constraints on Afterglow Models from Observations of the Early-Time Radio Evolution

43 citations · 99 across the 18 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

Emission line formation in scattering dominated media: implications for LRDs

Elisha Modelevsky, Omri Nitzan, Re'em Sari +1

Recent JWST observations of ``Little Red Dots'' (LRDs) reveal broad and prominent Balmer emission lines. We present a theoretical framework for intrinsic emission line formation an…

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

Dynamics in Nuclear Stellar Clusters: The Impact of Collisions and Disrupted Binaries

Barak Rom, Re'em Sari

The nuclear stellar clusters surrounding supermassive black holes (SMBHs) host millions of stars and stellar remnants. We study how stellar collisions and binary disruptions, along…

astro-ph.GA2026

The - Relation Has to Break

Omri Nitzan, Re'em Sari

We revisit the growth of central black holes via tidal disruption events (TDEs) and plunges of stellar-mass black holes (sBHs). Our model incorporates the current understanding of…

astro-ph.GA2024★ 18 cited

Dynamics around supermassive black holes: Extreme mass-ratio inspirals as gravitational-wave sources

Barak Rom, Itai Linial, Karamveer Kaur +1

Supermassive black holes and their surrounding dense stellar environments nourish a variety of astrophysical phenomena. We focus on the distribution of stellar-mass black holes aro…