The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays (2008)

First Author: Sesana A

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2008.13682.x

Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2008.13682.x

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1