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离子化气体在一个奇怪的无线电圈宿主星系中延伸超过40Kpc
Alison L Coil1, Serena Perrotta2, David S N Rupke3
1Department of Astronomy and Astrophysics, University of California, La Jolla, CA, USA. acoil@ucsd.edu.
Nature
|January 9, 2024
概括
奇怪的无线电圈 (ORC) 是一个神秘的天文物体. 显微镜数据显示中心银河系中的电离气体,
科学领域:
- 银河系外的天文学
- 银河系的演变
- 宇宙现象
背景情况:
- 奇特的无线电圈 (ORCs) 是新发现的银河系外无线电源,其特点是具有大,微弱,扩散的无线电发射环.
- ORCs的起源仍然未知,尽管相关的星系具有红移,表明它们的射电结构具有很大的物理尺度.
研究的目的:
- 通过分析ORC4中中心星系的光谱数据来研究ORC的性质.
- 要确定来自中心星系的光学辐射与ORC的大规模无线电辐射有关.
主要方法:
- 在ORC4中获取和分析中心星系的光谱数据.
- 测量了电离气体的范围,速度梯度,速度分散和[O II]等效宽度.
主要成果:
- 在ORC4的中心星系中检测到来自电离气体的强烈[O II]辐射,z=0.4512.
- [O II] 辐射跨度约为40 kpc,显示速度梯度和高速度分散,对于静止的星系来说,其相当宽度非常高.
- 观察到的形态,动力学和发射强度与向外移动的冲击后的冲击电离气体一致.
结论:
- 观测到的[O II]辐射表明银河系附近发生了一场戏剧性事件,
- ORC 的扩展光学和无线电辐射都可能来自同一个能量事件,尽管它们的尺度大不相同.
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