Internal magnetic fields of pulsars, white dwarfs, and other stars

Details Internal magnetic fields of pulsars, white dwarfs, and other stars Internal magnetic fields of pulsars, white dwarfs, and other stars

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...195..751o&link_type=abstract

Astrophysical Journal, vol. 195, Feb. 1, 1975, pt. 1, p. 751, 752.

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3

Magnetic Field Configurations, Pulsars, Stellar Interiors, Stellar Magnetic Fields, White Dwarf Stars, Astronomical Models, Electrical Resistivity, Magnetic Effects, Mathematical Models, Stellar Structure, Supernovae

Scientific paper

The possibility that the very early magnetic fields in pulsars and other stars have a large number of nodes in the radial function, has been considered by some authors. However, these analyses have not taken into account the fact that this large number of nodes implies large internal magnetic fields. Such large fields could affect the interior dynamics and may also give rise to stability problems.

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