一颗以716赫兹旋转的无线电脉冲星
Jason W T Hessels1, Scott M Ransom, Ingrid H Stairs
1Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada. hessels@physics.mcgill.ca
概括
天文学家在Terzan 5球状星团中发现了一颗716赫兹的阴影二进制射电脉冲星. 这一发现揭示了迄今为止旋转速度最快的中子星,挑战了现有的恒星进化模型和最大旋转速率.
科学领域:
- 天文学和天体物理学
- 紧的对象 紧的对象
- 中子星是什么意思 中子星是什么意思
背景情况:
- 中子星是大质量恒星的残余,以极端密度和快速旋转而闻名.
- 脉冲星是旋转的中子星,它们会发射出电磁辐射.
- 球状星团是密集的恒星集合,常常容纳异国情调的恒星群体.
研究的目的:
- 发现和描述快速旋转的中子星.
- 测试关于中子星最大自旋速率的理论.
- 为了研究脉冲星在密集的恒星环境中的特性.
主要方法:
- 使用绿岸望远镜进行无线电观测.
- 通过它们的周期性无线电辐射检测脉冲星.
- 分析轨道参数和流量密度,以对照二进制星系.
主要成果:
- 在球状星团Terzan 5中发现了一颗716赫兹阴影二进制射电脉冲星.
- 这颗脉冲星是有记录以来旋转速度最快的中子星,超过了之前的记录.
- 低流量密度和高日食分数表明存在更快的脉冲星.
结论:
- 这颗脉冲星的快速旋转率挑战了限制中子星旋转的模型.
- 它的特性为中子星半径和质量理论提供了约束.
- 这一发现突显了在球状星团中发现更极端物体的潜力.
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