Geodetic Precession and the Binary Pulsar B1913+16

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dc.creatorKarastergiou, A.
dc.creatorKramer, M.
dc.creatorWex, N.
dc.creatorvon Hoensbroech, A.
dc.date2000-02-04
dc.date.accessioned2026-07-07T01:52:07Z
dc.date.available2026-07-07T01:52:07Z
dc.descriptionA 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.
dc.description2 pages, 1 figure, IAU 177 Colloquium: Pulsar Astronomy - 2000 and Beyond
dc.identifierhttps://arxiv.org/abs/astro-ph/0002099
dc.identifierhttp://arxiv.org/abs/astro-ph/0002099
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/516
dc.subjectAstrophysics
dc.titleGeodetic Precession and the Binary Pulsar B1913+16
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