主动性星系尘埃散射锥偏振的建模
天体物理学
2007-05-23 v1
摘要
我们采用 STOKES 辐射传递代码，对主动性星系（AGN）极端区域的尘埃散射引起的偏振进行建模。我们讨论在 optical/UV 波段对不同观察角度下，两种不同类型尘埃（一种为银河尘埃模型，另一种为 AGN 灰度推断的尘埃模型）的光谱强度和偏振的波长依赖性。STOKES 代码及其文档可在 http://www.stokes-program.info/ 免费获取。
引用
@article{arxiv.astro-ph/0701163,
title = {Modeling the Polarization of Dusty Scattering Cones in Active Galactic Nuclei},
author = {Rene W. Goosmann and C. Martin Gaskell and M. Shoji},
journal= {arXiv preprint arXiv:astro-ph/0701163},
year = {2007}
}
备注
2 pages, 1 figure, conference proceedings of the AGN meeting held in October 2006 in Xi'an, China. To appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M. Wang (San Francisco: ASP)