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这是异常X射线脉冲星4U0142+61的光学对应物
F Hulleman1, M H van Kerkwijk, S R Kulkarni
1Astronomical Institute, Utrecht University, The Netherlands. f.hulleman@astro.uu.nl
Nature
|December 29, 2000
概括
异常X射线脉冲星 (AXP) 的能量来源仍然未知. 深度光学观测表明4U0142+61附近的一个奇特的物体是对应物体,可能由磁性磁层辐射提供动力.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
背景情况:
- 异常的X射线脉冲星 (AXPs) 缺乏明确的能量来源,与典型的脉冲星或增积双星不同.
- 标准的能量损失机制 (旋转能量,积累) 不足以为AXP提供动力.
- 关于AXP能量来源的两个主要假设是积累盘或磁铁磁场衰变.
研究的目的:
- 为了研究异常X射线脉冲星 (AXP) 的能量来源.
- 为了识别最亮的AXP的光学对应物,4U0142+61.
- 为了区分AXP能源的积累盘和磁铁模型.
主要方法:
- 对围绕AXP 4U0142+61.61的场进行深度光学观测.
- 分析光学对应的位置和颜色.
- 观察到的光学辐射与理论模型的比较.
主要成果:
- 在4U0142+61.1.的精确位置检测到一个异常光学颜色的物体.
- 光学辐射太微弱,无法支持大型积累盘模型.
- 观察到的光学辐射与来自磁星的磁层辐射一致.
结论:
- 识别的光学物体很可能是AXP 4U0142+61.61的对应物.
- 这些发现有利于磁星模型,表明能量源于磁场衰变.
- 需要进一步的多波长观测来确认AXP的性质.
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