Free precession of neutron stars: role of possible vortex pinning.
Abstract
Vortex pinning affects neutron-star free precession by modifying its frequency and geometry, in a gyroscopic effect. For neutron stars with low oblateness, the free-precession frequency is given by the product of the ratio of moments of inertia of the pinned superfluid to the rigid component of the rest of the star times half the superfluid vorticity. This poses a severe difficulty for any interpretation of the 35-day cycle of Her X-1 in terms of neutron-star wobble if vortex pinning exists.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- May 1977
- DOI:
- 10.1086/155249
- Bibcode:
- 1977ApJ...214..251S
- Keywords:
-
- Moments Of Inertia;
- Neutron Stars;
- Precession;
- Stellar Models;
- Stellar Rotation;
- Angular Velocity;
- Binary Stars;
- Ideal Fluids;
- Magnus Effect;
- Vorticity;
- X Ray Sources;
- Astronomy