Fig. 2 from Flare X‐Ray Observations of AB Doradus: Evidence of Stellar Coronal Opacity

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Flare X‐Ray Observations of AB Doradus: Evidence of Stellar Coronal Opacity

Authors: M. Matranga, M. Mathioudakis, H. R. M. Kay, and F. P. Keenan

Matranga et al. 2005 The Astrophysical Journal Letters 621 L125.

Provider: AAS Journals

Caption: Fig. 2.

Observed spectrum (solid line), predicted spectrum (dashed line), and continuum (dotted line) of the flare. The predicted spectrum has been calculated using the new atomic calculation of Doron & Behar (2002). The wavelength grid of the predicted spectrum has been shifted by 0.1 Å for clarity. The observed overpredicted ratio for the Fe XVII 15.01 Å line is lower compared to the quiescent state.

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