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constraint that the
total magnetic charge must be zero. In 2005, Yu. V.
Glagolevskij modeled the
field as a
dipole displaced from the star's center, and inclined...
-
sight for an
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Glagolevskij and G. A.
Chuntonov examined the
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Properties of Main
Sequence Magnetic Stars". Astrophysical...
-
Centre de données
astronomiques de Strasbourg.
Retrieved 30
October 2024.
Glagolevskij, Yu. V. (2019). "On
Properties of Main
Sequence Magnetic Stars". Astrophysical...
