Modeling light echoes from hot dust and the broad line region in Active Galactic Nuclei

模拟来自热尘埃和活动星系核中宽线区域的光回波

• 批准号: 2009508
• 负责人: Andrew Robinson
• 金额: $ 37.13万
• 依托单位: Rochester Institute of Tech
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2020
• 资助国家: 美国
• 起止时间: 2020-09-01 至 2024-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2009508&HistoricalAwards=false
• 关键词: Modeling; light; echoes; hot; dust

We now know that most galaxies in the universe host a supermassive black hole at their centers. As interstellar gas falls in towards the black hole, a huge amount of energy is released, creating an extremely bright light source at the center of the galaxy. These sources, called Active Galactic Nuclei, can far outshine the galaxy’s entire population of stars. Because inter-galactic distances are vast, Active Galactic Nuclei are difficult to resolve even using the best images obtained with current telescopes. However, by measuring “light echoes” astronomers can probe the environment around the black hole. In this project, the PI will develop a computer program to model these light echoes. By comparing computer generated “echo maps” with data obtained from several observational surveys, the PI will be able to map the gas and dust structures in large numbers of Active Galactic Nuclei. A series of Astronomy and Physics Days for local high school students will be hosted at the RIT campus, which will include talks and activities specifically designed to address the interests and concerns of female students. The broad emission lines observed in the spectra of Active Galactic Nuclei provide key diagnostics of various physical properties, including the mass of the black hole. The inner region (the “central engine”) is surrounded by a torus of dusty molecular gas. This structure obscures our observations and severely hinders studies of the black hole growth phase. Due to their distances, Active Galactic Nuclei are difficult to study by direct imaging with current telescopes. However, an alternative method, known as reverberation mapping, can be used. The broad emission lines and the infrared emission from dust embedded in the torus respond to variations in the central engine’s luminosity with a delay due to light travel times. This produces a “light echo” that contains information on the spatial distribution, velocity field and other properties of the emitting gas and dust. In this project, the PI will develop a computer code to produce detailed models of the light echoes of both the broad emission lines and the infrared emission from the torus dust. The PI will use the code to model data from several current and near future observational reverberation mapping surveys. By modeling these data sets, the PI aims to map the gas and dust structures in large samples of Active Galactic Nuclei. This will help characterize the evolution of the supermassive black hole population over cosmic time. Upon completion of the project, the computer code and related products, such as the computed echo maps, will be made available to the scientific community.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

我们现在知道，宇宙中大多数星系的中心都有一个超大质量黑洞。当星际气体福尔斯落入黑洞时，释放出大量的能量，在星系中心产生了一个非常明亮的光源。这些被称为活动星系核的光源，可以远远超过星系中所有的恒星。由于星系间的距离是巨大的，即使使用目前望远镜获得的最好的图像，活动星系核也很难分辨。然而，通过测量“光回波”，天文学家可以探测黑洞周围的环境。在这个项目中，PI将开发一个计算机程序来模拟这些光回波。通过比较计算机生成的“回波图”与从几次观测调查中获得的数据，PI将能够绘制大量活动星系核中的气体和尘埃结构。将在RIT校园为当地高中学生举办一系列天文学和物理学日活动，其中包括专门为解决女学生的兴趣和关切而设计的讲座和活动。在活动星系核的光谱中观察到的宽发射线提供了各种物理性质的关键诊断，包括黑洞的质量。内部区域（“中央引擎”）被尘埃分子气体环所包围。这种结构模糊了我们的观察，严重阻碍了对黑洞生长阶段的研究。由于它们的距离，活动星系核很难用现有的望远镜直接成像来研究。然而，可以使用称为混响映射的替代方法。宽的发射线和嵌入在环面中的尘埃的红外发射响应于中央引擎的光度变化，由于光的传播时间而延迟。这会产生一个“光回波”，其中包含了关于空间分布、速度场和发射气体和尘埃的其他属性的信息。在这个项目中，PI将开发一个计算机代码，以产生来自环形尘埃的宽发射线和红外发射的光回波的详细模型。PI将使用该代码对当前和不久的将来的几次观测混响映射调查的数据进行建模。通过对这些数据集进行建模，PI的目标是绘制活动星系核大样本中的气体和尘埃结构。这将有助于描述超大质量黑洞种群在宇宙时间内的演化特征。项目完成后，计算机代码和相关产品，如计算的回波图，将提供给科学界。该奖项反映了NSF的法定使命，并已被认为是值得通过使用基金会的智力价值和更广泛的影响审查标准进行评估的支持。