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Possibility of Detecting Moons of Pulsar Planets through Time-of-Arrival Analysis

Lewis, Karen; Sackett, Penny; Mardling, Rosemary Anne

Description

The perturbation caused by planet-moon binarity on the time-of-arrival signal of a pulsar with an orbiting planet is derived for the case in which the orbits of the moon and the planet-moon barycenter are both circular and coplanar. The signal consists of two sinusoids with frequency (2np-3nb) and (2np-nb), where np and nb are the mean motions of the planet and moon around their barycenter, and the planet-moon system around the host, respectively. The amplitude of the signal is the fraction sin...[Show more]

CollectionsANU Research Publications
Date published: 2008
Type: Journal article
URI: http://hdl.handle.net/1885/31932
Source: Astrophysical Journal, The
DOI: 10.1086/592743

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