Image Details
Caption: Figure 8.
Left: evolution of the spectral break and power-law slopes from the RATAN radio light curve (V. A. Allakhverdyan et al. 2024). Right: for clarity, we plot with fainter points all epochs where the uncertainties of the slopes are larger than 0.2. Two characteristic fits of radio spectra from individual epochs are presented.
© 2026. The Author(s). Published by the American Astronomical Society.