首页> 外文OA文献 >Non-LTE Models and Theoretical Spectra of Accretion Disks in Active Galactic Nuclei II. Vertical Structure of the Disk
【2h】

Non-LTE Models and Theoretical Spectra of Accretion Disks in Active Galactic Nuclei II. Vertical Structure of the Disk

机译:非LTE模型和活动中吸积盘的理论谱  银河核II。磁盘的垂直结构

摘要

We have calculated several representative models of vertical structure of anaccretion disk around a supermassive Kerr black hole. The interaction ofradiation and matter is treated self-consistently, taking into accountdepartures from LTE for calculating both the disk structure and the radiationfield. The structural equations are described in detail, and variousapproximations are discussed. We have demonstrated that departures from LTE arevery important for determining the disk structure, even at the midplane, aswell as the emergent radiation, particularly for hot and electron--scattering--dominated disks. We have shown that at least for the disk parameters studied inthis paper, NLTE effects tend to reduce the value of the Lyman jump withrespect to the LTE predictions, regardless whether LTE predicts an emission orabsorption jump. We have studied the effects of various values of viscosity onthe model structure and predicted spectral energy distribution. The viscosityis parameterized through a parameter $lpha_0$ which describes thevertically-averaged viscous stress, two power-law exponents $zeta_0$ and$zeta_1$, and the division point $m_{d}$ between these two forms. The diskstructure and emergent radiation is sensitive mainly to the values of$lpha_0$, while the other parameters influence the disk structure to a muchlesser extent. However, although the detailed shape of the predicted spectrumis sensitive to adopted value of $lpha_0$, the overall appearance of thespectrum is quite similar.
机译:我们已经计算了围绕超大质量克尔黑洞的吸积盘垂直结构的几种代表性模型。考虑到LTE的偏差,同时计算了磁盘结构和辐射场,因此辐射与物质的相互作用得到了自洽的处理。详细描述结构方程,并讨论各种近似。我们已经证明,偏离LTE对于确定磁盘结构,甚至在中平面以及出现的辐射非常重要,特别是对于以热和电子散射为主的磁盘而言。我们已经证明,至少对于本文研究的磁盘参数,相对于LTE预测,NLTE效果往往会降低莱曼跳变的值,而无论LTE是否预测发射跳变或吸收跳变。我们研究了各种粘度值对模型结构和预测光谱能量分布的影响。通过描述垂直平均粘性应力的参数$ alpha_0 $,两个幂律指数$ zeta_0 $和$ zeta_1 $以及这两种形式之间的分界点$ m_ {d} $来对粘度进行参数化。磁盘结构和出射辐射主要对$ alpha_0 $的值敏感,而其他参数对磁盘结构的影响程度要小得多。但是,尽管预测频谱的详细形状对$ alpha_0 $的采用值敏感,但频谱的整体外观非常相似。

著录项

  • 作者

    Hubeny I.; Hubeny V.;

  • 作者单位
  • 年度 1998
  • 总页数
  • 原文格式 PDF
  • 正文语种
  • 中图分类

相似文献

  • 外文文献
  • 中文文献
  • 专利

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号