隐藏NGC 1068黑洞的尘埃的热成像
Violeta Gámez Rosas1, Jacob W Isbell2, Walter Jaffe3
1Leiden Observatory, Leiden University, Leiden, Netherlands. gamez@strw.leidenuniv.nl.
Nature
|February 17, 2022
概括
通过NGC 1068的新中红外图像再次证实了活跃星系核的统一模型. 这些图像显示中央发动机被厚厚的边缘磁盘所掩盖,在最近的修改中支持原始模型.
科学领域:
- 天文学与天体物理学
- 银河系的演变
- 观测宇宙学
背景情况:
- 统一模型解释了活跃星系核 (AGN) 的分类,该分类基于一个中心黑洞周围的尘土的方向.
- 最近的高分辨率图像挑战了这个模型,
- 这种重新解释需要为2型AGN分类提供临时解释.
研究的目的:
- 研究2型星系NGC1068的结构和尘埃分布.
- 测试统一模型的有效性与最近的替代解释.
- 为AGN中的遮蔽提供新的观测证据.
主要方法:
- 获取和分析NGC 1068的多频段中红外图像.
- 在银河系内绘制尘埃温度分布图.
- 整合新的无线电数据以确定中央发动机的位置 (正在编写的手稿).
主要成果:
- 新的红外图像证实了中心发动机周围有一个厚厚的,几乎边缘的遮蔽盘.
- 中心发动机位于之前报告的环形特征下方.
- 确定了极流的排放和吸尘的独特矿物质特性.
结论:
- 这些发现重申了AGN分类的原始统一模型.
- 厚厚的边缘仍然是2型AGN的主要遮蔽结构.
- 这项研究强调了多波长观测对于理解AGN的重要性.
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