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Glagolevskij, Yu. V.; Betrix, F. (1997). "Properties of He-rich stars. I.
Their evolutionary...
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Glagolevskij, Yu. V. (2019). "On
Properties of Main
Sequence Magnetic Stars". Astrophysical...
-
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
observer on the Earth, as the star rotates. In 2007, Yu. V.
Glagolevskij and G. A.
Chuntonov examined the
extensive data
which had been collected...
-
Centre de données
astronomiques de Strasbourg.
Retrieved 30
October 2024.
Glagolevskij, Yu. V. (2019). "On
Properties of Main
Sequence Magnetic Stars". Astrophysical...
-
Centre de données
astronomiques de Strasbourg.
Retrieved 15
October 2024.
Glagolevskij, Yu. V. (2019). "On
Properties of Main
Sequence Magnetic Stars". Astrophysical...
- Bibcode:2017MNRAS.468.2745N, doi:10.1093/mnras/stx674, S2CID 119215348.
Glagolevskij, Yu. V. (2019), "On
Properties of Main
Sequence Magnetic Stars", Astrophysical...
- 116 (1): 284–292, Bibcode:1998AJ....116..284E, doi:10.1086/300413.
Glagolevskij, Yu. V. (January 2019). "On
Properties of Main
Sequence Magnetic Stars"...
-
varied in
antiphase with the
ionized chromium lines. In 1981, Y. V.
Glagolevskij measured a
large magnetic field of CQ UMa,
interpreting it to be variable...
- 1134/S1063773712050015. eISSN 1562-6873. ISSN 1063-7737. S2CID 119257644.
Glagolevskij, Yu. V. (January 2019). "On
Properties of Main
Sequence Magnetic Stars"...