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
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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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