Woan, G. (2005) Gravitoastronomy with neutron stars. In: Gravitational Wave and Particle Astrophysics Detectors, Glasgow, Scotland, 23 June 2004, (doi: 10.1117/12.550057)
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Woan4784SPIE.pdf 678kB |
Publisher's URL: http://dx.doi.org/10.1117/12.550057
Abstract
Recent advances in gravitational wave detectors mean that we can start to make astrophysically important statements about the physics of neutron stars based on observed upper limits to their gravitational luminosity. Here we consider statements we can already make about a selection of known radio pulsars, based on data from the LIGO and GEO600 detectors, and look forward to what could be learned from the first detections.
Item Type: | Conference Proceedings |
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Keywords: | Gravitational waves, pulsars, neutron stars, LIGO, GEO600. |
Status: | Published |
Refereed: | Yes |
Glasgow Author(s) Enlighten ID: | Woan, Professor Graham |
Authors: | Woan, G. |
Subjects: | Q Science > QB Astronomy |
College/School: | College of Science and Engineering > School of Physics and Astronomy |
Research Centre: | College of Science and Engineering > School of Physics and Astronomy > Institute for Gravitational Research |
Publisher: | SPIE |
ISSN: | 0277-786X |
Copyright Holders: | Copyright © 2005 SPIE |
First Published: | First published in Proceedings of SPIE 5500:(49) |
Publisher Policy: | Reproduced in accordance with the copyright policy of the publisher |
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