Pulsar magnetogyro ratios and pulsar evolution. III - Magnetic field generation

Details Pulsar magnetogyro ratios and pulsar evolution. III - Magnetic field generation Pulsar magnetogyro ratios and pulsar evolution. III - Magnetic field generation

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...279..803w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 279, April 15, 1984, p. 803-806.

Astronomy and Astrophysics

Astrophysics

6

Gyromagnetism, Hall Effect, Pulsars, Stellar Evolution, Stellar Magnetic Fields, Magnetohydrodynamics, Stellar Models, Stellar Rotation

Scientific paper

The relationship between period (P) and magnetogyro ratio (gamma) is examined for a sample of 293 pulsars from the catalog of Manchester and Taylor (1981), and an evolutionary scheme based on the thermally driven Hall limited-field battery effect (Woodward; 1978, 1982) is proposed for pulsars with P less than about 500 msec. A P/gamma diagram is shown, and the independence of gamma (at about 1.6 x 10 to the -8th) from P in these the short-period pulsars is demonstrated. Only neutron-star models based on stiff equations of state are found to give plausible results in this scheme.

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