Chemo-dynamical modelling with Schwarzschild's method | |
Long, Richard John2,3; Mao, Shude1,2,3,4 | |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
2018-12-01 | |
卷号 | 18期号:12页码:8 |
关键词 | galaxies: abundances galaxies: formation galaxies: individual (NGC 1248, NGC 3838, NGC 4452, NGC 4551) galaxies: kinematics and dynamics galaxies: structure methods: numerical |
ISSN号 | 1674-4527 |
DOI | 10.1088/1674-4527/18/12/145 |
英文摘要 | We extend Schwarzschild's dynamical modelling method to model absorption line strength data as well as the more usual luminosity and kinematic data. Our approach draws on earlier published work by the first author with the Syer & Tremaine made-to-measure (M2M) dynamical modelling method and uses similar ideas to create a chemo-Schwarzschild method. We apply our extended Schwarzschild method to the same four early type galaxies (NGC 1248, NGC 3838, NGC 4452, NGC 4551) as the chemo-M2M work, and are able to recover successfully the 2D absorption line strength for the three lines we model (H beta, Fe5015, Mg b). We believe that this is the first time Schwarzschild's method has been used in this way. The techniques developed can be applied to modelling other aspects of galaxies, for example age and metallicity data coming from stellar population modelling, and are not specific to absorption line strength data. |
资助项目 | National Key Basic Research and Development Program of China[2018YFA0404501] ; National Natural Science Foundation of China[11333003] ; National Natural Science Foundation of China[11390372] ; National Natural Science Foundation of China[11761131004] |
WOS关键词 | GALAXY ; IV |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
WOS记录号 | WOS:000454953800001 |
资助机构 | National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/24321] |
专题 | 中国科学院国家天文台 |
通讯作者 | Long, Richard John |
作者单位 | 1.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China 3.Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England 4.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China |
推荐引用方式 GB/T 7714 | Long, Richard John,Mao, Shude. Chemo-dynamical modelling with Schwarzschild's method[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2018,18(12):8. |
APA | Long, Richard John,&Mao, Shude.(2018).Chemo-dynamical modelling with Schwarzschild's method.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,18(12),8. |
MLA | Long, Richard John,et al."Chemo-dynamical modelling with Schwarzschild's method".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 18.12(2018):8. |
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