Published July 1, 1988
| Version v1
Journal article
The large glitch from PSR 0355+54 and its post-glitch relaxation
- 1. Scientific and Technical Research Council of Turkey, Kocaeli. Research Inst. for Basic Sciences
- 2. Illinois Univ., Urbana (USA). Dept. of Physics
- 3. Columbia Univ., New York (USA). Columbia Astrophysics Lab.
- 4. Columbia Univ., New York (USA). Dept. of Physics
Description
The recently observed large glitch of PSR 0355 + 54 and its post-glitch relaxation are interpreted within the vortex creep model applied previously to the post-glitch timing data for the Crab and Vela pulsars and for PSR 0525 + 21. A linear response regime of vortex creep is shown to explain the post-glitch observations and is likely to be operative in parts of the neutron star crust superfluid. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 233
- Journal Issue
- 1
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 25-31
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 19102635
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CREEP; MATHEMATICAL MODELS; NEUTRON STARS; PULSARS; RADIOWAVE RADIATION; RELAXATION TIME; ROTATION; TIME DEPENDENCE; TRANSIENTS; VORTICES
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; MECHANICAL PROPERTIES; RADIATIONS; STARS