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Millimeter-Wave Monitoring of Active Galactic Nuclei with the Africa Millimetre Telescope

机译:非洲毫米波望远镜对活跃银河核的毫米波监测

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Active galactic nuclei are the dominant sources of gamma rays outside our galaxy and are also candidates for the source of ultra-high energy cosmic rays. In addition to being emitters of broad-band non-thermal radiation throughout the electromagnetic spectrum, their emission is highly variable on timescales from years to minutes. Hence, high-cadence monitoring observations are needed to understand their emission mechanisms. The Africa Millimetre Telescope is planned to be the first mm-wave radio telescope on the African continent and one of few in the southern hemisphere. Further to contributing to the global mm-VLBI observations with the Event Horizon Telescope, substantial amounts of observation time will be available for monitoring observations of active galactic nuclei. Here we review the scientific scope of the Africa Millimetre Telescope for monitoring of active galactic nuclei at mm-wavelengths.
机译:活跃的银河核是我们银河系以外伽马射线的主要来源,也是超高能宇宙射线来源的候选者。除了是整个电磁频谱中的宽带非热辐射的发射器之外,它们的发射在数年至数分钟的时间范围内也是高度可变的。因此,需要高节奏的监测观测来了解其排放机理。非洲毫米望远镜计划成为非洲大陆上的第一台毫米波射电望远镜,也是南半球为数不多的毫米波射电望远镜之一。除了通过事件地平线望远镜为全球mm-VLBI观测做出贡献之外,还将有大量的观测时间可用于监视活动银河核的观测。在这里,我们回顾了非洲毫米望远镜在毫米波波长下监测活动银河核的科学范围。

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