Amanote Research

Amanote Research

    RegisterSign In

Post-Newtonian Dynamical Modeling of Supermassive Black Holes in Galactic-Scale Simulations

Astrophysical Journal - United States
doi 10.3847/1538-4357/aa6d65
Full Text
Open PDF
Abstract

Available in full text

Categories
AstrophysicsAstronomyPlanetary ScienceSpace
Date

May 4, 2017

Authors
Antti RantalaPauli PihajokiPeter H. JohanssonThorsten NaabNatalia LahénTill Sawala
Publisher

American Astronomical Society


Related search

LISA Observations of Supermassive Black Holes: Parameter Estimation Using Full Post-Newtonian Inspiral Waveforms

Physical Review D
2008English

Large Scale Direct Galaxy Collision Simulations With Central Supermassive Binary Black Holes

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Supermassive Black Holes, Large Scale Structure and Holography

Journal of Modern Physics
2013English

Observational Evidence for Supermassive Black Holes

Symposium - International Astronomical Union
1989English

Supermassive Black Holes Then and Now

1998English

Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-Ray Background

English

Disks Around Merging Binary Black Holes: From GW150914 to Supermassive Black Holes

Physical Review D
AstronomyPhysics
2018English

Formation of the First Supermassive Black Holes

English

Gravitational Wave Background From Supermassive Black Holes

2011English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy