一颗巨大的恒星具有足够强大的磁场形成磁星
Tomer Shenar1, Gregg A Wade2, Pablo Marchant3
1Anton Pannekoek Institute for Astronomy, University of Amsterdam, 1098 XH Amsterdam, Netherlands.
概括
研究人员在HD 45166系统中发现了一颗具有强磁场的沃尔夫-雷耶恒星. 预计这颗恒星在超新星爆炸后会形成磁星,一种高度磁化的中子星.
科学领域:
- * 天体物理学
- * 恒星进化
- * 中子星形成
背景情况:
- *磁星是具有极强磁场的中子星, 但它们的起源尚不清楚.
- * 沃尔夫-雷耶恒星是热的,富含的恒星,其特征在于光谱中的辐射线.
- 对于天体物理学来说, 了解像磁星这样的奇特恒星残骸的形成途径至关重要.
研究的目的:
- 为了研究二进制星系HD 45166的性质.
- * 为了确定系统中的沃尔夫-雷耶星的属性.
- 为了探索磁星的潜在形成机制.
主要方法:
- * 对HD 45166系统的光谱测定.
- *对二进制系统的存档轨道数据进行重新分析.
- * 恒星演变模型和计算
主要成果:
- * HD 45166 系统拥有一个质量为 2 个太阳质量的 Wolf-Rayet 恒星.
- 在沃尔夫-雷耶星上检测到43千高斯的显著磁场.
- * 恒星进化预测表明超新星爆炸导致磁星残留物.
结论:
- * 观察到的沃尔夫-雷耶星具有足够的磁场强度来形成磁星.
- *这颗磁化的沃尔夫-雷耶恒星的可能形成场景是两个质量较低的恒星的合并.
- 这项研究提供了巨大的恒星磁星形成的潜在途径.
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