activity
20092014
most citedObservational Signatures of Binary Supermassive Black Holes

134 citations · 134 across the 1 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2014★ 134 cited

Observational Signatures of Binary Supermassive Black Holes

Constanze Roedig, Julian H. Krolik, M. Coleman Miller

Observations indicate that most massive galaxies contain a supermassive black hole, and theoretical studies suggest that when such galaxies have a major merger, the central black h…

astro-ph.HE2013

Migration of massive black hole binaries in self--gravitating accretion discs: Retrograde versus prograde

Constanze Roedig, Alberto Sesana

We study the interplay between mass transfer, accretion and gravitational torques onto a black hole binary migrating in a self-gravitating, retrograde circumbinary disc. A direct c…

astro-ph.HE2012

General relativistic radiation hydrodynamics of accretion flows: II. Treating stiff source terms and exploring physical limitations

Constanze Roedig, Olindo Zanotti, Daniela Alic

We present the implementation of an implicit-explicit (IMEX) Runge-Kutta numerical scheme for general relativistic hydrodynamics coupled to an optically thick radiation field in tw…

astro-ph.CO2012

Evolution of binary black holes in self gravitating discs: dissecting the torques

Constanze Roedig, Alberto Sesana, Massimo Dotti +3

We study the interplay between gas accretion and gravity torques in changing a binary elements and its total angular momentum (L) budget. Especially, we analyse the physical origin…

astro-ph.CO2011

Origin and Implications of high eccentricities in massive black hole binaries at sub-pc scales

Constanze Roedig, Alberto Sesana

We outline the eccentricity evolution of sub-parsec massive black hole binaries (MBHBs) forming in galaxy mergers. In both stellar and gaseous environments, MBHBs are expected to g…

astro-ph.CO2011

Multimessenger astronomy with pulsar timing and X-ray observations of massive black hole binaries

A. Sesana, C. Roedig, M. T. Reynolds +1

We demonstrate that very massive (>10^8\msun), cosmologically nearby (z<1) black hole binaries (MBHBs), which are primary targets for ongoing and upcoming pulsar timing arrays (PTA…