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超新星亮度的光学耀斑持续数分钟

Anna Y Q Ho1, Daniel A Perley2, Ping Chen3

  • 1Department of Astronomy, Cornell University, Ithaca, NY, USA. annayqho@cornell.edu.

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概括

天文学家从AT2022tsd中观察到快速的光学耀斑, 这表明它是一个强大的,紧的能量源. 这一发现支持了一些外星系光学瞬态被磁星或积聚黑洞所驱动的观点.

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科学领域:

  • 天文学与天体物理学
  • 高能天体物理学
  • 短暂的事件

背景情况:

  • 仅持续几天的外星系光学瞬态不同于典型的超新星.
  • 像牛一样的瞬态物体呈现出蓝色和强烈的无线电/X射线辐射,暗示着独特的能量来源.
  • 之前的观察表明,AT2018具有类似牛的能量来源,包括X射线变异性和紫外线辐射.

研究的目的:

  • 调查AT2018牛状过渡性AT2022tsd的性质.
  • 描述AT2022TSD事件之后的能量现象.
  • 确认这些瞬态物体的存在和类型.

主要方法:

  • 在几个月内从AT2022tsd观测光学耀斑.
  • 对耀斑持续时间,能量和光谱属性的分析.
  • 与已知的短暂现象和理论模型进行比较.

主要成果:

  • 在AT2022tsd之后发现了持续数分钟的光学耀斑.
  • 这些火焰具有高度的能量,
  • 证据表明来自短暂源的流出或喷射接近相对论.

结论:

  • 观察到的耀斑证实了AT2022像牛一样的短暂的能量来源.
  • 能量来源很可能是磁星或增长的黑洞.
  • 这些发现有助于我们更好地理解短暂的外星系光学瞬态.