Fig. 1 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. 1.

AB Dor light curve derived from EPIC‐pn using a bin size of 200 s. During the observation, two flares were observed. The flare and quiescent time intervals (FLARE and QUIES1+QUIES2, respectively) used to extract the RGS spectra are shown. Times in seconds since JD 2,450,814.0.

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