论文标题
检测具有当前和未来调查的中quaSar中的中间质量黑洞
Detecting intermediate mass black holes in midiquasars with current and future surveys
论文作者
论文摘要
缺乏检测到的中间质量黑洞在我们对天体物理对物体最奇特的生长和演变的理解方面构成了差距。在这里，我们研究了矮星系中心中间质量黑洞发射的低亮度相对论喷气机的可能性。我们建立了人口模型，使我们能够对他们的无线电排放进行预测，并通过当前和将来的调查来量化其可检测性。我们发现，即将在SKA，NGVLA和Vera C. Rubin天文台（如SKA和无线电）中使用的仪器，如果存在，则可能能够检测出这些来源人群的大量部分（$> 38 \％$）。此外，我们的结果表明，由于现有的调查可能已经检测到了低亮度活跃的银河系核可能已经检测到的少量中quiquasars可能不会伪装。
The lack of detected intermediate mass black holes poses a gap in our understanding of the growth and evolution of the most exotic of astrophysical objects. Here we investigate the possibility of low-luminosity relativistic jets launched by intermediate mass black holes in the centers of dwarf galaxies. We built population models that allow us to make predictions for their radio emission and quantify their detectability by current and future surveys. We find that the upcoming instruments in optical and radio like the SKA, ngVLA and the Vera C. Rubin Observatory will likely be able to detect a significant fraction ($>38\%$) of such sources population if they exist. In addition, our results suggest that it is not unlikely a small number of midiquasars possibly masquerading as low-luminosity active galactic nuclei may have already been detected by existing surveys.
