18 citations · 56 across the 17 of their papers we have counts for
6 papers · 1 filter
Evolution of Main Sequence Stars Transferring Mass to a Supermassive Black Hole
Andrey Sandomirsky, Re'em Sari, Aleksandra Olejak +1
We consider main-sequence stars orbiting close to a supermassive black hole (SMBH), which are potential gravitational wave (GW) sources for LISA if their orbital periods are of the…
Mass Segregation and Transient Formation in Nuclear Stellar Clusters
Barak Rom, Re'em Sari
Supermassive black holes at the centers of galaxies occasionally disrupt stars or consume stellar-mass black holes (BHs) that wander too close, producing observable electromagnetic…
Semi-Analytical Fokker Planck Models for Nuclear Star Clusters
Karamveer Kaur, Barak Rom, Re'em Sari
We study the dynamics of nuclear star clusters, the dense stellar environments surrounding massive black holes in the centers of galaxies. We consider angular momentum diffusion du…
Self-similarity of the third type in ultra relativistic blastwaves
Tamar Faran, Andrei Gruzinov, Re'em Sari
A new type of self-similarity is found in the problem of a plane-parallel, ultra-relativistic blast wave, propagating in a powerlaw density profile of the form . S…
Formation of Merging Stellar-Mass Black Hole Binaries by Gravitational Wave Emission in Active Galactic Nucleus Disks
Barak Rom, Re'em Sari, Dong Lai
Many stellar-mass Black Holes (sBHs) are expected to orbit supermassive black holes at galactic centers. For galaxies with Active Galactic Nuclei (AGN), it is likely that the sBHs…
Evolution of Supernova Remnants near the Galactic Center
Almog Yalinewich, Tsvi Piran, Re'em Sari
Supernovae near the galactic center evolve differently from regular galactic supernovae. This is mainly due to the environment into which the supernova remnants propagate. Instead…