中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Cautionary remarks on using SPH to model the ISM in galaxies

文献类型:期刊论文

作者Williams, PR; Churches, DK; Nelson, AH; Duc, PA; Braine, J; Brinks, E
刊名RECYCLING INTERGALACTIC AND INTERSTELLAR MATTER
出版日期2004
期号217页码:226-227
英文摘要In many SPH simulations of galaxy formation a lower limit is imposed on the kernel radius h equal to the gravitational softening length e. It has been found that such a constraint can in some circumstances compromise the spatial resolution to which hydrodynamical quantities are evaluated to the extent that the evolution of the gross features of a numerical galaxies are affected. Such effects can be avoided by allowing h to evolve freely to maintain a roughly constant number of neighbours in SPH summations. Here we focus on how imposing a constraint on h may affect the velocity field.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
收录类别SCI ; ISTP
语种英语
WOS记录号WOS:000222682600058
源URL[http://119.78.226.72/handle/331011/19368]  
专题上海天文台_星系宇宙学重点实验室
作者单位Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
推荐引用方式
GB/T 7714
Williams, PR,Churches, DK,Nelson, AH,et al. Cautionary remarks on using SPH to model the ISM in galaxies[J]. RECYCLING INTERGALACTIC AND INTERSTELLAR MATTER,2004(217):226-227.
APA Williams, PR,Churches, DK,Nelson, AH,Duc, PA,Braine, J,&Brinks, E.(2004).Cautionary remarks on using SPH to model the ISM in galaxies.RECYCLING INTERGALACTIC AND INTERSTELLAR MATTER(217),226-227.
MLA Williams, PR,et al."Cautionary remarks on using SPH to model the ISM in galaxies".RECYCLING INTERGALACTIC AND INTERSTELLAR MATTER .217(2004):226-227.

入库方式: OAI收割

来源:上海天文台

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