Bert Vander Meulen, P. Camps, Djordje Savic, M. Baes, Giorgio Matt, M. Stalevski
{"title":"X-ray polarisation in AGN circumnuclear media. Polarisation framework and 2D torus models","authors":"Bert Vander Meulen, P. Camps, Djordje Savic, M. Baes, Giorgio Matt, M. Stalevski","doi":"10.1051/0004-6361/202450773","DOIUrl":null,"url":null,"abstract":"Cold gas and dust reprocess the central X-ray emission of active galactic nuclei (AGN), producing characteristic spectro-polarimetric features in the X-ray band. The recent launch of IXPE allows for observations of this X-ray polarisation signal, which encodes unique information on the parsec-scale circumnuclear medium of obscured AGN. However, the models for interpreting these polarimetric data are under-explored and do not reach the same level of sophistication as the corresponding spectral models. We aim at closing the gap between the spectral and spectro-polarimetric modelling of AGN circumnuclear media in the X-ray band by providing the tools for simulating X-ray polarisation in complex geometries of cold gas alongside X-ray spectra. We lay out the framework for X-ray polarisation in 3D radiative transfer simulations and provide an implementation to the 3D radiative transfer code SKIRT, focussing on (de)polarisation due to scattering and fluorescent re-emission. As an application, we explored the spectro-polarimetric properties of a 2D toroidal reprocessor of cold gas, modelling the circumnuclear medium of AGN. For the 2D torus model, we find a complex behaviour of the polarisation angle with photon energy, which we interpret as a balance between the reprocessed photon flux originating from different sky regions, with a direct link to the torus geometry. We calculated a large grid of AGN torus models and demonstrated how spatially resolved X-ray polarisation maps could form a useful tool for interpreting the geometrical information that is encoded in IXPE observations. With this work, we release high-resolution AGN torus templates that simultaneously describe X-ray spectra and spectro-polarimetry for observational data fitting with XSPEC. The SKIRT code can now model X-ray polarisation simultaneously with X-ray spectra and provide synthetic spectro-polarimetric observations for complex 3D circumnuclear media, with all features of the established SKIRT framework available.","PeriodicalId":8585,"journal":{"name":"Astronomy & Astrophysics","volume":"7 34","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-08-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1051/0004-6361/202450773","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Cold gas and dust reprocess the central X-ray emission of active galactic nuclei (AGN), producing characteristic spectro-polarimetric features in the X-ray band. The recent launch of IXPE allows for observations of this X-ray polarisation signal, which encodes unique information on the parsec-scale circumnuclear medium of obscured AGN. However, the models for interpreting these polarimetric data are under-explored and do not reach the same level of sophistication as the corresponding spectral models. We aim at closing the gap between the spectral and spectro-polarimetric modelling of AGN circumnuclear media in the X-ray band by providing the tools for simulating X-ray polarisation in complex geometries of cold gas alongside X-ray spectra. We lay out the framework for X-ray polarisation in 3D radiative transfer simulations and provide an implementation to the 3D radiative transfer code SKIRT, focussing on (de)polarisation due to scattering and fluorescent re-emission. As an application, we explored the spectro-polarimetric properties of a 2D toroidal reprocessor of cold gas, modelling the circumnuclear medium of AGN. For the 2D torus model, we find a complex behaviour of the polarisation angle with photon energy, which we interpret as a balance between the reprocessed photon flux originating from different sky regions, with a direct link to the torus geometry. We calculated a large grid of AGN torus models and demonstrated how spatially resolved X-ray polarisation maps could form a useful tool for interpreting the geometrical information that is encoded in IXPE observations. With this work, we release high-resolution AGN torus templates that simultaneously describe X-ray spectra and spectro-polarimetry for observational data fitting with XSPEC. The SKIRT code can now model X-ray polarisation simultaneously with X-ray spectra and provide synthetic spectro-polarimetric observations for complex 3D circumnuclear media, with all features of the established SKIRT framework available.
冷气体和尘埃会对活动星系核(AGN)的中心 X 射线辐射进行再处理,从而在 X 射线波段产生特征性的光谱极化特征。最近发射的 IXPE 允许对这种 X 射线偏振信号进行观测,它编码了关于被遮挡 AGN 的等秒尺度环核介质的独特信息。然而,用于解释这些偏振数据的模型还未得到充分探索,其复杂程度也无法与相应的光谱模型相提并论。我们的目标是缩小 AGN 环核介质在 X 射线波段的光谱和光谱极坐标建模之间的差距,提供在复杂的冷气体几何结构中模拟 X 射线极化的工具,同时提供 X 射线光谱。我们制定了三维辐射传递模拟中的 X 射线极化框架,并提供了三维辐射传递代码 SKIRT 的实施方案,重点是散射和荧光再发射引起的(去)极化。作为一项应用,我们探索了冷气体二维环形后处理器的光谱偏振特性,模拟了 AGN 的环核介质。对于二维环状模型,我们发现偏振角随光子能量变化的复杂行为,我们将其解释为来自不同天空区域的再处理光子通量之间的平衡,这与环状几何形状有直接联系。我们计算了一个大网格的 AGN 环形模型,并展示了空间分辨 X 射线偏振图如何成为解释 IXPE 观测所编码的几何信息的有用工具。通过这项工作,我们发布了高分辨率 AGN 环形模板,这些模板可同时描述 X 射线光谱和光谱极化,用于 XSPEC 的观测数据拟合。现在,SKIRT 代码可以同时对 X 射线偏振和 X 射线光谱进行建模,并为复杂的三维环核介质提供合成光谱偏振观测数据,同时提供已建立的 SKIRT 框架的所有功能。