Amanote Research

Amanote Research

    RegisterSign In

Constraints on the Dynamical Environments of Supermassive Black-Hole Binaries Using Pulsar-Timing Arrays

Physical Review Letters - United States
doi 10.1103/physrevlett.118.181102
Full Text
Open PDF
Abstract

Available in full text

Categories
AstronomyPhysics
Date

May 3, 2017

Authors
Stephen R. TaylorJoseph SimonLaura Sampson
Publisher

American Physical Society (APS)


Related search

Supermassive Black Hole Binaries at High Energies

International Journal of Modern Physics: Conference Series
2014English

Testing General Relativity With Black Hole-Pulsar Binaries

Physical Review D
AstronomyPhysics
2018English

Massive Black Hole Binaries: Dynamical Evolution and Observational Signatures

Advances in Astronomy
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Black Hole Pulsar

Physical Review D
AstronomyPhysics
2018English

Super-Massive Black Hole Binaries in Gas-Rich Environments

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Possible Observational Signatures of Supermassive Black Hole Binaries in Their Fe Kα Line Profiles

Contributions of the Astronomical Observatory Skalnate Pleso
AstrophysicsAstronomy
2020English

Testing General Relativity Using Golden Black-Hole Binaries

Physical Review D
AstronomyPhysics
2016English

Pulsar Timing Arrays and the Cosmological Constant

2014English

The Supermassive Black Hole at the Galactic Center

Annual Review of Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy