在棕色矮星周围存在辐射带的证据
J B Climent1,2, J C Guirado1,3, M Pérez-Torres4,5
1Departament d'Astronomia i Astrofísica, Universitat de València, E-46100 Burjassot Spain.
概括
超冷矮星具有与木星相似的磁场,具有辐射带和极光. 这些发现是基于对棕矮星LSR J1835+3259的详细无线电观测.
科学领域:
- 天文学与天体物理学
- 星球科学
背景情况:
- 超冷矮星包括棕矮星和非常低质量的恒星.
- 无线电观测通过光曲线和光谱能量分布提供了UCD磁场的洞察力.
研究的目的:
- 用空间分辨率的无线电观测来研究棕矮星LSR J1835+3259的磁场结构.
- 确定UCD是否具有类似辐射带的结构和相关现象.
主要方法:
- 采用非常长的基线干涉测量来对LSR J1835+3259进行高分辨率无线电观测.
- 分析了扩展无线电发射的形态,并与理论模型进行了比较.
主要成果:
- 空间分辨率的无线电观测显示了LSR J1835+3259的扩展无线电发射.
- 观测到的无线电发射形态与含有能量粒子的辐射带相一致.
结论:
- 无线电发射UCD可能具有双极排序的磁场.
- 这些磁场产生了类似于辐射带的形态和极光,类似于在木星上观察到的.
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