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Quiescent and Flaring States of Three Active Stars: V834 Tau, LQ Hya, and BY Dra

  • Authors: Gurpreet Singh, Jeewan C. Pandey, Subhajeet Karmakar

Gurpreet Singh et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 3.

Evolution of spectral parameters with time. The first panel of each plot shows the variation of X-ray luminosity in the F band. The second and third panels show the evolution of the temperatures and corresponding emission measures (EMs). Here, green and blue represent the hot and cool quiescent components, respectively, while purple denotes the flaring components. The last panel shows the variation of the average coronal abundances with time.

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