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The activity of young star
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The activity of young star
Contents
Introduction
About solar physics. The chromosphere, arch structure of corona, the local magnetic field and solar activity
Forecasts, forecasts … The transition from the Sun to the stars, convection and heating of the plasma in the outer atmosphere, stellar winds and cooling crowns
X-rays of stellar coronas. The stars of early spectral classes, the expected maximum of the F-Star, two-level of X-rays of red dwarfs, communication with the axial rotation
Active – means young. From protostars to the main sequence stars, stage of stars of T Tau, the connection of X-rays with age, hinges in stellar coronas, slowing the rotation of the stellar wind
The chromosphere and the transition to the crown. Short-wave radiation of stars, the cycles of activity, activity in the chromosphere and transition region from the chromosphere to the corona, the expiry of the substance in the late giants and supergiants
Outbreaks of the stars. Features of outbreaks, physics of pulse phenomena, flare at the giant, briefly about radio emission from stars of late spectral classes
Conclusion
Literature
Кацова М.М., Лившиц М.А. Активность молодых звезд. – М.: Знание, 1986. – 64 с.