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Detection of Oscillations in a Type I X-Ray Burst of 4U 0614+091 with SVOM/ECLAIRs

  • Authors: Sébastien Le Stum, Floriane Cangemi, Alexis Coleiro, Sébastien Guillot, Jérôme Chenevez, Philippe Bacon, Nicolas Bellemont, Laurent Bouchet, Tristan Bouchet, Cécile Cavet, Bertrand Cordier, Antoine Foisseau, Olivier Godet, Andrea Goldwurm, Xuhui Han, Cyril Lachaud, Zhaosheng Li, Huali Li, Yulei Qiu, Jérôme Rodriguez, Wenjun Tan, Lian Tao, Lauryne Verwaerde, Chenwei Wang, Jing Wang, Jianyan Wei, Chao Wu, Wenjin Xie, Liping Xin, Shaolin Xiong, Shuangnan Zhang, Shijie Zheng

Sébastien Le Stum et al 2026 The Astrophysical Journal Letters 997 .

  • Provider: AAS Journals

Caption: Figure 5.

Upper limit of the orbital periods set by the Δν (dashed lines) and ﹩\dot{\nu }﹩ (solid lines) as a function of MWD, at different inclinations i, and for MNS = 1.2 (left) and MNS = 2.0 M⊙ (right). The areas of the parameter space incompatible with the hypothesis that both Δν and ﹩\dot{\nu }﹩ originate from orbital motion are represented in gray.

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