SIMBAD references

2021MNRAS.507L..36L - Mon. Not. R. Astron. Soc., 507, L36-L40 (2021/October-2)

Generating neutron-star magnetic fields: three dynamo phases.

LANDER S.K.

Abstract (from CDS):

Young neutron stars (NSs) have magnetic fields in the range 1012-1015 G, believed to be generated by dynamo action at birth. We argue that such a dynamo is actually too inefficient to explain the strongest of these fields. Dynamo action in the mature star is also unlikely. Instead we propose a promising new precession-driven dynamo and examine its basic properties, as well as arguing for a revised mean-field approach to NS dynamos. The precession-driven dynamo could also play a role in field generation in main-sequence stars.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): dynamo - stars: evolution - stars: magnetic field - stars: neutron - stars: rotation

Simbad objects: 3

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