Spectral Energy Distribution of Ultraluminous X-ray Sources from X-ray to the Optical Range

被引：0
|
作者：
Vinokurov, A. [1 ]
Atapin, K. [1 ,2 ]
Fabrika, S. [1 ]
机构：
[1] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz, Russia
[2] Lomonosov Moscow State Univ, Sternberg Astron Inst, Moscow, Russia
来源：
STARS: FROM COLLAPSE TO COLLAPSE | 2017年 / 510卷
基金：
俄罗斯基础研究基金会; 俄罗斯科学基金会;
关键词：
COMPTONIZATION MODELS; BLACK-HOLES;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We model spectral energy distributions (SEDs) of ultraluminous X-ray sources (ULXs) using Shakura and Sunyaev's approach to a supercritical accretion disk. We consider a funnel in the supercritical accretion disk and wind arising in the funnel. The wind is illuminated by funnel radiation and it reprocesses the radiation to the UV and optical ranges. We take into account Comptonization of a hot corona which covers inner parts of the supercritical disk. We apply the model to a typical ultraluminous X-ray source Holmberg II X-1.
引用
收藏
页码：476 / 477
页数：2
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