在磁星SGR 1900+14周围的一个红外环
S Wachter1, E Ramirez-Ruiz, V V Dwarkadas
1Spitzer Science Center, California Institute of Technology, Pasadena, California 91125, USA. wachter@ipac.caltech.edu
Nature
|May 30, 2008
概括
天文学家发现磁星SGR 1900+14周围有一个红外环. 这一环支持了磁星起源于大质量恒星的理论,并由巨大的耀斑形成.
科学领域:
- 天文学和天体物理学
- 高能天体物理学 高能天体物理学
- 中子星物理学 中子星物理学
背景情况:
- 磁星是具有非常强磁场的中子星,与无线电脉冲星不同.
- 以前的研究表明磁星和巨大的祖先恒星之间存在联系.
- 磁星和其他中子星之间的进化关系仍然不清楚.
研究的目的:
- 为了研究围绕磁星SGR 1900+14.的红外环的性质.
- 为了确定观察到的环状结构的起源和形成机制.
- 为了巩固磁星和大质量恒星之间的联系.
主要方法:
- 使用红外成像对磁星SGR 1900+14的观测.
- 对戒指的形态,尺寸和能量进行分析.
- 观测数据与恒星演变和磁性耀斑的理论模型的比较.
主要成果:
- 在磁星SGR 1900+14周围发现了一个圆的红外环或外.
- 环的特征与标准的恒星质量损失或超新星残留进化不一致.
- 1998年由巨大的磁星耀斑所造成的无尘空洞的理论模型准确地预测了环的尺寸.
结论:
- 观察到的红外环很可能是磁星SGR 1900+14发出的巨型耀斑的结果.
- 这一发现为SGR 1900+14与一群大质量恒星星团的联系提供了有力的证据.
- 这项研究巩固了磁星和巨大的恒星祖先之间的联系.
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