中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
ON THE INFLUENCE OF MINOR MERGERS ON THE RADIAL ABUNDANCE GRADIENT IN DISKS OF MILKY-WAY-LIKE GALAXIES

文献类型:期刊论文

作者Zinchenko, Igor A.1,2; Berczik, Peter1,2,3; Grebel, Eva K.2; Pilyugin, Leonid S.1,2,4; Just, Andreas2
刊名ASTROPHYSICAL JOURNAL
出版日期2015-06-20
卷号806期号:2
关键词galaxies: abundances galaxies: evolution galaxies: kinematics and dynamics
英文摘要We investigate the influence of stellar migration caused by minor mergers (mass ratio from 1: 70 to 1: 8) on the radial distribution of chemical abundances in the disks of Milky-Way-like galaxies during the last 4 Gyr. A GPU-based pure N-body tree-code model without hydrodynamics and star formation was used. We computed a large set of mergers with different initial satellite masses, positions, and orbital velocities. We find that there is no significant metallicity change at any radius of the primary galaxy in the case of the accretion of a low-mass satellite of 10(9) M-circle dot (mass ratio 1: 70) except for the special case of a prograde satellite motion in the disk plane of the host galaxy. The accretion of a satellite of mass >= 3 x 10(9) M-circle dot (mass ratio 1: 23) results in an appreciable increase of the chemical abundances at galactocentric distances larger than similar to 10 kpc. The radial abundance gradient flattens in the range of galactocentric distances from 5 to 15 kpc in the case of a merger with a satellite with mass. 3 x 109 M.. There is no significant change in the abundance gradient slope in the outer disk (from similar to 15 kpc up to 25 kpc) in any merger while the scatter in metallicities at a given radius significantly increases for most of the satellite's initial masses/positions compared to the case of an isolated galaxy. This argues against attributing the break (flattening) of the abundance gradient near the optical radius observed in the extended disks of Milky-Way-like galaxies only to merger-induced stellar migration.
收录类别SCI
语种英语
WOS记录号WOS:000357129500122
源URL[http://ir.bao.ac.cn/handle/114a11/5655]  
专题国家天文台_星系宇宙学研究部
作者单位1.Natl Acad Sci Ukraine, Main Astron Observ, UA-03680 Kiev, Ukraine
2.Heidelberg Univ, Zentrum Astron, Astron Rechen Inst, D-69120 Heidelberg, Germany
3.Chinese Acad Sci, Natl Astron Observ China, Beijing 1000128, Peoples R China
4.Kazan Fed Univ, Kazan 420008, Russia
推荐引用方式
GB/T 7714
Zinchenko, Igor A.,Berczik, Peter,Grebel, Eva K.,et al. ON THE INFLUENCE OF MINOR MERGERS ON THE RADIAL ABUNDANCE GRADIENT IN DISKS OF MILKY-WAY-LIKE GALAXIES[J]. ASTROPHYSICAL JOURNAL,2015,806(2).
APA Zinchenko, Igor A.,Berczik, Peter,Grebel, Eva K.,Pilyugin, Leonid S.,&Just, Andreas.(2015).ON THE INFLUENCE OF MINOR MERGERS ON THE RADIAL ABUNDANCE GRADIENT IN DISKS OF MILKY-WAY-LIKE GALAXIES.ASTROPHYSICAL JOURNAL,806(2).
MLA Zinchenko, Igor A.,et al."ON THE INFLUENCE OF MINOR MERGERS ON THE RADIAL ABUNDANCE GRADIENT IN DISKS OF MILKY-WAY-LIKE GALAXIES".ASTROPHYSICAL JOURNAL 806.2(2015).

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来源:国家天文台

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