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.
We conducted three observations of the periastron passages of DQ Tau using X-ray telescopes: in 2010 , 2021 , and 2022 . Notably, significant X-ray flares were detected on all three occasions. In Figure 8, we compare the duration, peak X-ray luminosity, and energetics of these DQ Tau flares with numerous large X-ray flares produced by young stars, as studied by Getman et al. and Getman & Feigelson .
We conducted three observations of the periastron passages of DQ Tau using X-ray telescopes: in 2010 , 2021 , and 2022 . Notably, significant X-ray flares were detected on all three occasions. In Figure 8, we compare the duration, peak X-ray luminosity, and energetics of these DQ Tau flares with numerous large X-ray flares produced by young stars, as studied by Getman et al. and Getman & Feigelson .
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