Geodetic Precession and the Binary Pulsar B1913+16
ArXiv astro-ph/0002099 (2000)
Abstract:
A change of the component separation in the profiles of the binary pulsar PSR B1913+16 has been observed for the first time (Kramer 1998) as expected by geodetic precession. In this work we extend the previous work by accounting for recent data from the Effelsberg 100-m telescope and Arecibo Observatory and testing model predictions. We demonstrate how the new information will provide additional information on the solutions of the system geometry.Geodetic precession and the binary pulsar B1913+16
PULSAR ASTRONOMY - 2000 AND BEYOND: IAU COLLOQUIUM 177 202 (2000) 125-126
Identification of physical components in pulsar emission
PULSAR ASTRONOMY - 2000 AND BEYOND: IAU COLLOQUIUM 177 202 (2000) 177-178