activity
20062012
most citedDynamical evolution of the young stars in the Galactic center: N-body simulations of the S-stars

102 citations · 350 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2012★ 41 cited

Stellar Energy Relaxation around A Massive Black Hole

Ben Bar-Or, Gábor Kupi, Tal Alexander

[abridged] Energy relaxation around a massive black hole (MBH) is key to establishing the dynamical state of galactic nuclei, and the nature of close stellar interactions with the…

gr-qc2011★ 27 cited

Galactic rotation curves in brane world models

L. Á. Gergely, T. Harko, M. Dwornik +2

In the braneworld scenario the four dimensional effective Einstein equation has extra source terms, which arise from the embedding of the 3-brane in the bulk. These non-local effec…

astro-ph.GA2009★ 102 cited

Dynamical evolution of the young stars in the Galactic center: N-body simulations of the S-stars

Hagai B. Perets, Alessia Gualandris, Gabor Kupi +2

We use N-body simulations to study the evolution of the orbital eccentricities of stars deposited near (<0.05 pc) the Milky Way massive black hole (MBH), starting from initial cond…

astro-ph2008★ 1 cited

Dynamical evolution of the young stars in the Galactic center

Hagai. B. Perets, Alessia Gualandris, David Merritt +1

Recent observations of the Galactic center revealed a nuclear disk of young OB stars near the massive black hole (MBH), in addition to many similar outlying stars with higher eccen…

astro-ph2008★ 72 cited

The efficiency of resonant relaxation around a massive black hole

Ehud Eilon, Gábor Kupi, Tal Alexander

Resonant relaxation (RR) is a rapid relaxation process that operates in the nearly-Keplerian potential near a massive black hole (MBH). RR dominates the dynamics of compact remnant…

astro-ph2007★ 3 cited

Determination of the upper and lower bound of masslimit of degenerate fermionic dark matter objects

Gábor Kupi

We give a gravitational upper limit for the mass of static degenerate fermionic dark matter objects. The treatment we use includes fully relativistic equations for describing the s…