In this paper, researchers conducted NuSTAR, Swift, and Chandra observations on the DQ Tau high-eccentricity binary system to confirm the presence of X-ray supe
This paper is available on arxiv under CC 4.0 license. Authors: Konstantin V. Getman, Department of Astronomy & Astrophysics, Pennsylvania State University; Agnes Kospal, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, E¨otv¨os Lor´and Research Network , MTA Centre of Excellence, Max Planck Institute for Astronomy, and ELTE E¨otv¨os Lor´and University, Institute of Physics; Nicole Arulanantham, Space Telescope Science Institute; Dmitry A.
Drawing upon recent observations conducted during a single orbit of DQ Tau in July-August 2022, which utilized NuSTAR, Swift, and Chandra telescopes , alongside previously gathered X-ray and mm-band data from multiple periastrons of DQ Tau , our study embarks on an extensive analysis to compute the energetic characteristics of X-ray/NUV/optical flares within DQ Tau . Serendipitously, we discovered X-ray super-flares outside of periastron, potentially related to interacting magnetospheres .
Drawing upon recent observations conducted during a single orbit of DQ Tau in July-August 2022, which utilized NuSTAR, Swift, and Chandra telescopes , alongside previously gathered X-ray and mm-band data from multiple periastrons of DQ Tau , our study embarks on an extensive analysis to compute the energetic characteristics of X-ray/NUV/optical flares within DQ Tau . Serendipitously, we discovered X-ray super-flares outside of periastron, potentially related to interacting magnetospheres .
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