Expected evolution of disk wind properties along an x-ray binary outburst

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• who: Petrucci P.-O. et al. from the UnivGrenoble Alpes, CNRS, IPAG, Grenoble, France Villanova University, Department of Physics, Villanova, PA, USA have published the research work: Expected evolution of disk wind properties along an X-ray binary outburst, in the Journal: (JOURNAL)
• what: While GX 339-4 never showed signatures of hot wind in the X-rays the dataset used is optimal for the analysis shown in this study. The authors show that the disk wind can transit from stable to unstable states for Fe XXV and Fe XXVI ions on day timescale. The . . .
  

   

  

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