A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf
.
FAST STELLAR PULSATIONS AND LOCAL MAGNETIC FIELDS
БЫСТРЫЕ ЗВЕЗДНЫЕ ПУЛЬСАЦИИ И ЛОКАЛЬНЫЕ МАГНИТНЫЕ ПОЛЯ
2020
Proceedings of the 24th All-Russia Conference on Solar and Solar-Terrestrial Physics
unpublished
БЫСТРЫЕ ЗВЕЗДНЫЕ ПУЛЬСАЦИИ И ЛОКАЛЬНЫЕ МАГНИТНЫЕ ПОЛЯ
The results of studies by of superfast (on minute and second scales) line profile variability in spectra of early-type star are reviewed. The spectra of program OBA stars were obtained with the 6-meter BTA telescope using a multi-mode SCORPIO reducer and using the MSS spectrograph with an exposure of 1-150 seconds and a total observation time of 2-3 hours. The variability of the line profiles is analyzed. Regular variations of the H, HeI, FeII, NII, OII, SiII line profiles were detected in
doi:10.31725/0552-5829-2020-317-320
fatcat:rdqjqkjabfcevffc4kdcwrnbyi