Atoms in magnetic fields: possible origin of chemical anomalies in magnetic stars.

Details Atoms in magnetic fields: possible origin of chemical anomalies in magnetic stars. Atoms in magnetic fields: possible origin of chemical anomalies in magnetic stars.

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002oap....15...11b&link_type=abstract

Odessa Astronomical Publications, v. 15, p. 11-15.

Astronomy and Astrophysics

Astronomy

Stars: Atomic Magnetic Moments, Magnetic Stars.

Scientific paper

The interaction of atomic magnetic moments with non-uniform magnetic fields may be important for the diffusion in the matter near the surface of neutron and magnetic stars. Formation of the anomalous abundance of some elements in magnetic stars is considered as an extension of the old model of Babcock (1963) and Jensen (1962). Phase transition of the second order is shown to be held in helium as a transition from diamagnetic to paramagnetic stare with increasing of magnetic field (Bisnovatyi-Kogan and Hoflich, 1990), efficiency.

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