在SS 433中,来自扩展的X射线喷射的铁排放线:原子核的再加热
Simone Migliari1, Rob Fender, Mariano Méndez
1Astronomical Institute "Anton Pannekoek," University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, Netherlands. migliari@astro.uva.nl
概括
研究人员使用Chandra观测研究了X射线二进制 (XRB) SS 433的X射线喷射. 他们在喷气中发现了现场再加热和相对论速度的证据.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- 黑洞物理学 黑洞物理学
背景情况:
- 相对论喷流是与增加的黑洞和中子星相关的能量现象.
- 尽管进行了广泛的研究,但这些喷气的结构和组成仍然不太清楚.
- 射线二进制 (XRBs) 提供了一个附近的实验室,用于研究喷气形成和进化.
研究的目的:
- 研究来自X射线二进制星SS 433的相对论喷流的结构和组成.
- 为了分析SS 433喷气机的空间分辨率的X射线光谱数据.
- 了解喷气中发生的物理过程,例如再加热和粒子加速.
主要方法:
- 利用Chandra先进的电荷合器件成像光谱仪进行X射线光谱.
- 进行了弧度二级X射线喷射的空间分辨率分析.
- 分析了光谱特征,包括连续发射和多普勒移排放线.
主要成果:
- 在喷射的空间分辨率区域中检测到热连续和多普勒转移的铁排放线.
- 提供了在现场重新加热喷气式飞机的微子元件的证据.
- 确认相对论散体速度在喷气式飞机发射后持续超过100天.
结论:
- 这项研究揭示了相对论喷流中正在进行的物理过程,挑战了关于它们演变的先前假设.
- 在现场再加热是维持喷气材料高能量和温度的重要机制.
- 这些发现为X射线二进制星体中的增积驱动喷气的复杂动力学提供了新的见解.
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