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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
DOI10.1088/1674-4527/18/12/145
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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