Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-27T22:54:55.743Z Has data issue: false hasContentIssue false
  • English
  • Français

Neutron star seismology

Published online by Cambridge University Press:  20 March 2013

Nils Andersson
Nils Andersson*
Affiliation:
University of Southampton, United Kingdom email: na@maths.soton.ac.uk
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

I will provide an overview of recent improvements in our models for vibrating neutron stars, discussing the role of composition, heat, crust elasticity and superfluidity. I will explain how the results may impact on observations, in particular related to magnetar QPOs and future gravitational-wave searches.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 159
Copyright
Copyright © International Astronomical Union 2013