activity
19972024
most citedOptical and Radio Properties of Extragalactic Sources Observed by the FIRST and SDSS Surveys

517 citations · 9.2k across the 122 of their papers we have counts for

collaborators
Showing 1998Show all

6 papers · 1 filter

astro-ph1998★ 65 cited

Structure and properties of transition fronts in accretion discs

Kristen Menou, Jean-Marie Hameury, Rudolf Stehle

We use high-resolution time-dependent numerical simulations of accretion discs around white dwarfs to study the structure and properties of transition fronts in the context of the…

astro-ph1998★ 52 cited

A Population of Faint Non-Transient Low Mass Black Hole Binaries

Kristen Menou, Ramesh Narayan, Jean-Pierre Lasota

We study the thermal and viscous stability of accretion flows in Low Mass Black Hole Binaries (LMBHBs). We consider a model in which an inner advection-dominated accretion flow (AD…

astro-ph1998★ 65 cited

On the Cosmological Evolution of the Luminosity Function and the Accretion Rate of Quasars

Zoltan Haiman, Kristen Menou

We consider a class of models for the redshift evolution (between $0\lsim z \lsim 4$) of the observed optical and X-ray quasar luminosity functions (LFs), with the following assump…

astro-ph1998★ 232 cited

Black Hole and Neutron Star Transients in Quiescence

Kristen Menou, Ann A. Esin, Ramesh Narayan +3

We consider the X-ray luminosity difference between neutron star and black hole soft X-ray transients (NS and BH SXTs) in quiescence. The current observational data suggest that BH…

astro-ph1998★ 102 cited

Accretion disc outbursts: a new version of an old model

Jean-Marie Hameury, Kristen Menou, Guillaume Dubus +2

We have developed 1D time-dependent numerical models of accretion discs, using an adaptive grid technique and an implicit numerical scheme, in which the disc size is allowed to var…

gr-qc1998★ 4 cited

Astrophysical Evidence for Black Hole Event Horizons

Kristen Menou, Eliot Quataert, Ramesh Narayan

Astronomers have discovered many potential black holes in X-ray binaries and galactic nuclei. These black holes are usually identified by the fact that they are too massive to be n…