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19942024
most citedThermal Equilibria of Accretion Disks

603 citations · 1.6k across the 72 of their papers we have counts for

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13 papers · 1 filter

astro-ph2008★ 3 cited

The magneto-rotational instability near threshold: spatio-temporal amplitude equation and saturation

O. Regev

We show, by means of a perturbative weakly nonlinear analysis, that the axisymmetric magneto-rotational instability (MRI) in a magnetic Taylor-Couette (mTC) flow in a thin-gap give…

astro-ph2008★ 4 cited

Hydrodynamical activity in thin accretion disks

Oded Regev

An asymptotic treatment of thin accretion disks, introduced by Kluźniak & Kita (2000) for a steady-state disk flow, is extended to a time-dependent problem. Transient growth of axi…

astro-ph2007★ 56 cited

On the viability of the shearing box approximation for numerical studies of MHD turbulence in accretion disks

O. Regev, O. M. Umurhan

Most of our knowledge on the nonlinear development of the magneto-rotational instability (MRI) relies on the results of numerical simulations employing the shearing box (SB) approx…

astro-ph2007★ 1 cited

Chaos and complexity in astrophysics

Oded Regev

Methods and techniques of the theory of nonlinear dynamical systems and patterns can be useful in astrophysical applications. Some works on the subjects of dynamical astronomy, ste…

astro-ph2007★ 3 cited

Hydrodynamic response of rotationally supported flows in the Small Shearing Box model

A. Sternberg, O. M. Umurhan, Y. Gil +1

The hydrodynamic response of the inviscid small shearing box model of a midplane section of a rotationally supported astrophysical disk is examined. An energy functional …

astro-ph2007★ 24 cited

On the nonlinear saturation of the magnetorotational instability near threshold in a thin-gap Taylor-Couette setup

O. M. Umurhan, O. Regev, K. Menou

We study the saturation near threshold of the axisymmetric magnetorotational instability (MRI) of a viscous, resistive, incompressible fluid in a thin-gap Taylor-Couette configurat…

astro-ph2006★ 46 cited

A weakly nonlinear analysis of the magnetorotational instability in a model channel flow

O. M. Umurhan, K. Menou, O. Regev

We show by means of a perturbative weakly nonlinear analysis that the axisymmetric magnetorotational instability (MRI) of a viscous, resistive, incompressible rotating shear flow i…

astro-ph2005★ 1 cited

Hydrodynamical stability of thin accretion discs: transient growth of global axisymmetric perturbations

O. M. Umurhan, A. Nemirovsky, O. Regev +1

The purpose of this paper is to explore how accretion discs manifest the phenomenon of transient growth on a global scale. We investigate analytically the time response of a thin a…

astro-ph2004★ 120 cited

Hydrodynamic stability of rotationally supported flows: Linear and nonlinear 2D shearing box results

O. M. Umurhan, O. Regev

We present here both analytical and numerical results of hydrodynamic stability investigations of rotationally supported circumstellar flows using the shearing box formalism. Asymp…

astro-ph2003★ 19 cited

Launching jets from the boundary layer of accretion disks in young stellar objects

Noam Soker, Oded Regev

We reexamine a previously proposed model for thermal pressure acceleration of collimated outflows in young stellar objects (YSO). We are motivated by new results from recent X-ray…

astro-ph2002★ 36 cited

Asymptotic models of meridional flows in thin viscous accretion disks

O. Regev, L. Gitalman

We present the results of numerical integrations yielding the structure of and meridional flow in axisymmetric thin viscous accretion disk models. The solutions are obtained by sim…

astro-ph2001

On the effects of the stellar magnetic field on the structure of T Tauri accretion discs

Y. Ulchin, O. Regev, G. A. Wynn

The structure of accretion discs around magnetic T Tauri stars is numerically calculated using a particle hydrodynamical code, in which magnetic interaction is included in the fram…

astro-ph1994★ 603 cited

Thermal Equilibria of Accretion Disks

Marek A. Abramowicz, Xingming Chen, Shoji Kato +2

We show that most of hot, optically thin accretion disk models which ignore advective cooling are not self-consistent. We have found new types of optically thin disk solutions wher…