PMO OpenIR  > 太阳高能及相关物理过程研究团组
General relativistic magnetohydrodynamic and Monte Carlo Modeling of sagittarius A
Guy Hilburn ; Edison Liang ; Siming Liu ; Hui Li
2011
Source PublicationAstrophys Space Sci
ISSN1572-946X
Volume336Pages:145-149
AbstractWe present results of models of the physicalspace and parameters of the accretion disk of SagittariusA*, as well as simulations of its emergent spectrum. This begins with HARM, a 2D general relativistic magnetohydrodynamic(GRMHD) model, specifically set up toevolve the space around a black hole. Data from HARMare then fed into a 2D Monte-Carlo (MC) code which generatesand tracks emitted photons, allowing for absorptionand scattering before they escape the volume.Accretion disc ; Black hole;Galactic Center;Magnetohydrodynamics
KeywordAccretion Disc Black Hole Galactic Center Magnetohydrodynamics
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/4491
Collection太阳高能及相关物理过程研究团组
Recommended Citation
GB/T 7714
Guy Hilburn,Edison Liang,Siming Liu,et al. General relativistic magnetohydrodynamic and Monte Carlo Modeling of sagittarius A[J]. Astrophys Space Sci,2011,336:145-149.
APA Guy Hilburn,Edison Liang,Siming Liu,&Hui Li.(2011).General relativistic magnetohydrodynamic and Monte Carlo Modeling of sagittarius A.Astrophys Space Sci,336,145-149.
MLA Guy Hilburn,et al."General relativistic magnetohydrodynamic and Monte Carlo Modeling of sagittarius A".Astrophys Space Sci 336(2011):145-149.
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