布拉扎尔的电磁和引力辐射 OJ 287
Alexandr Volvach1, Larisa Volvach1, Mikhail Larionov2
1Radio Astronomy and Geodynamics Department of Crimean Astrophysical Observatory RAS, Katsively, Crimea.
iScience
|March 28, 2024
概括
通过使用天体力学和观测数据,开发了一种接近二进制超大质量黑洞 (SMBHs) 的新模型. 该模型确定了SMBH参数,揭示了OJ 287可能是最大的可比质量二进制SMBH.
科学领域:
- 天体物理学 天体物理学
- 宇宙学的宇宙学是什么?
- 黑洞物理学 黑洞物理学
背景情况:
- 星是由超大质量黑洞 (SMBHs) 驱动的活跃星系核.
- 了解二进制SMBH系统对于星系进化和引力波研究至关重要.
- OJ 287 是一个众所周知的黑星,被怀疑是二进制 SMBH 的宿主.
研究的目的:
- 提出一种新的模型来确定密切的二进制SMBH系统的参数.
- 分析二进制SMBH中的结构,动态和积累盘相互作用.
- 将OJ 287系统描述为一个潜在的大型二进制SMBH.
主要方法:
- 使用布拉撒长期监测数据 OJ 287.
- 运用天体力学定律进行轨道分析.
- 对无线电和光学观测数据进行和分析.
主要成果:
- 对二进制SMBH的确定质量,轨道元素和积累盘参数.
- 欧盟287号正式公布,被确定为具有可比质量的潜在最庞大的近距离二进制SMBH.
- 估计的引力波辐射,系统寿命和轨道变化.
结论:
- 拟议的模型有效地描述了二进制的SMBH系统.
- 欧盟287号公布了一个独特的实验室,用于研究大质量,可比质量的二进制SMBHs.
- 进一步的研究可以完善对引力波辐射和系统演变的预测.
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