J/MNRAS/269/849     Pulsar glitches (Alpar+ 1994)

Expectancy of large pulsar glitches: a comparison of models with the observed glitch sample Alpar M.A., Baykal A. <Mon. Not. R. Astron. Soc. 269, 849 (1994)> =1994MNRAS.269..849A 1994MNRAS.269..849A (SIMBAD/NED BibCode)
ADC_Keywords: Pulsars Keywords: MHD - stars: interiors - pulsars: general - stars: rotation Description: We study the expectancy of large glitches (ΔΩ/Ω>10^-7) from a sample of 430 pulsars other than the Vela pulsar. The pulsars in this sample have exhibited 19 large glitches. We assume that all pulsars experience such glitches, with rates that depend on the pulsar's rotation rate omega and spin-down rate omega, and on the glitch model. We use the core-quake model, and two variants of the superfluid vortex unpinning model, and choose model parameters such that the observed number of glitches is matched by the theoretically expected number. Among the models investigated, one of the superfluid vortex unpinning models gives good agreement with the observed distribution of glitches and with the parameter values deduced for the Vela pulsar glitches. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2 21 428 Time-spans of glitch-monitoring observations -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- PSR PSR name 10- 13 I4 d t Time-spans 15- 19 A5 --- Ref References (1) -------------------------------------------------------------------------------- Note (1): References: A : Ashworth & Lyne (1981MNRAS.195..517A 1981MNRAS.195..517A) B : Backus et al. (1982ApJ...255L..63B 1982ApJ...255L..63B) D : Downs G. S. (1982, private communication) G : Gullahom & Rankin (1978AJ.....83.1219G 1978AJ.....83.1219G) H : Helfand et al. (1980ApJ...237..206H 1980ApJ...237..206H) M : Manchester et al. (1983MNRAS.202..269M 1983MNRAS.202..269M) N : Newton et al. (1981, MNRAS 194, 841) (D) : Dewey et al. (1988ApJ...332..762D 1988ApJ...332..762D) (J) : Jones & Lyne (1988MNRAS.232..473J 1988MNRAS.232..473J) T : Taylor & Dewey (1988ApJ...332..770T 1988ApJ...332..770T) C : McConnell et al. (1991MNRAS.249..654M 1991MNRAS.249..654M) (G) : Gouiffes et al. (1992ApJ...394..581G 1992ApJ...394..581G) (JM): Johnston et al. (1992ApJ...387L..37J 1992ApJ...387L..37J) K : Kaspi et al. (1992ApJ...399L.155K 1992ApJ...399L.155K) S : Siegman, Manchester & Durdin (1993MNRAS.262..449S 1993MNRAS.262..449S) J : Johnston et al. (1995A&A...293..795J 1995A&A...293..795J) L : Lyne (private communication). -------------------------------------------------------------------------------- History: Prepared via OCR at CDS.
(End) James Marcout, Patricia Bauer [CDS] 01-Oct-1996
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