UDC 53
UDC 520
UDC 521
UDC 523
UDC 524
UDC 52-1
UDC 52-6
CSCSTI 41.00
CSCSTI 29.35
CSCSTI 29.31
CSCSTI 29.33
CSCSTI 29.27
CSCSTI 29.05
Russian Classification of Professions by Education 03.06.01
Russian Classification of Professions by Education 03.05.01
Russian Classification of Professions by Education 03.04.03
Russian Library and Bibliographic Classification 2
Russian Library and Bibliographic Classification 223
Russian Trade and Bibliographic Classification 614
Russian Trade and Bibliographic Classification 6135
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
The study of Be stars, characterized by emission lines and rotational velocities close to critical, has long been of interest to astrophysicists. These stars are distinguished by the presence of an equatorial disk, the formation mechanism of which remains unknown. To date, no magnetic field has been detected in any of these stars. The nature of the formation of Be star disks and their magnetism is still not well understood, and explaining them is one of the most urgent and complex problems in modern astrophysics. The star
stars: emission-line, Be, magnetic field; individual:
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