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Stellar population analysis on the stacked spectra of double-peaked emission-line galaxies
Wang, Meng-Xin1,2; Luo, A-Li1,2,3
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
2019-09-01
卷号19期号:9页码:18
关键词galaxies: evolution galaxies: stellar content
ISSN号1674-4527
DOI10.1088/1674-4527/19/9/126
英文摘要Double-peaked emission-line galaxies have long been perceived as objects related to merging galaxies or other phenomena with disturbed dynamical activities, such as outflows and disk rotation. In order to find the connection between the unique activities happening in these objects and their stellar population physics, we study the stellar populations of the stacked spectra drawn from double-peaked emission-line galaxies in the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 4 (DR4) and the Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) databases. We group the selected double-peaked emission-line objects into 10 different types of pairs based on the Baldwin-Phillips-Terlevich (BPT) diagnosis for each pair of blueshifted and redshifted components, and then stack the spectra of each group for analysis. The software STARLIGHT is employed to fit each stacked spectrum, and the contributions of stars at different ages and metallicities are quantified for subsequent comparative study and analysis. To highlight the commonality and uniqueness in these double-peaked emitting objects, we compare the population synthesis results of the stacked spectra of double-peaked emission-line galaxies with those of their counterpart reference samples displaying single-peaked emission features. The reference samples are also selected from the LAMOST DR4 and SDSS DR7 databases. From the comparison results, we confirm the strong correlations between stellar populations and their spectral classes, and find that the double-peaked emitting phenomenon is more likely to occur in an 'older' stellar environment and the subgroups hosting different BPT components will show an obvious heterogeneous star formation history.
资助项目National Natural Science Foundation of China (NSFC)[11603042] ; China Scholarship Council ; Brazilian agency CNPq ; Brazilian agency CAPES ; Brazilian agency FAPESP ; FranceBrazil CAPES/Cofecub program
WOS关键词ACTIVE-GALACTIC-NUCLEI ; DIGITAL SKY SURVEY ; EVOLUTIONARY SYNTHESIS ; SAURON PROJECT ; HOST GALAXIES ; NARROW LINES ; DATA RELEASE ; BLACK-HOLES ; CLASSIFICATION ; RESOLUTION
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:000485147000005
资助机构National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; China Scholarship Council ; China Scholarship Council ; Brazilian agency CNPq ; Brazilian agency CNPq ; Brazilian agency CAPES ; Brazilian agency CAPES ; Brazilian agency FAPESP ; Brazilian agency FAPESP ; FranceBrazil CAPES/Cofecub program ; FranceBrazil CAPES/Cofecub program ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; China Scholarship Council ; China Scholarship Council ; Brazilian agency CNPq ; Brazilian agency CNPq ; Brazilian agency CAPES ; Brazilian agency CAPES ; Brazilian agency FAPESP ; Brazilian agency FAPESP ; FranceBrazil CAPES/Cofecub program ; FranceBrazil CAPES/Cofecub program ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; China Scholarship Council ; China Scholarship Council ; Brazilian agency CNPq ; Brazilian agency CNPq ; Brazilian agency CAPES ; Brazilian agency CAPES ; Brazilian agency FAPESP ; Brazilian agency FAPESP ; FranceBrazil CAPES/Cofecub program ; FranceBrazil CAPES/Cofecub program ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; China Scholarship Council ; China Scholarship Council ; Brazilian agency CNPq ; Brazilian agency CNPq ; Brazilian agency CAPES ; Brazilian agency CAPES ; Brazilian agency FAPESP ; Brazilian agency FAPESP ; FranceBrazil CAPES/Cofecub program ; FranceBrazil CAPES/Cofecub program
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/27746]  
专题中国科学院国家天文台
通讯作者Luo, A-Li
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA
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GB/T 7714
Wang, Meng-Xin,Luo, A-Li. Stellar population analysis on the stacked spectra of double-peaked emission-line galaxies[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2019,19(9):18.
APA Wang, Meng-Xin,&Luo, A-Li.(2019).Stellar population analysis on the stacked spectra of double-peaked emission-line galaxies.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,19(9),18.
MLA Wang, Meng-Xin,et al."Stellar population analysis on the stacked spectra of double-peaked emission-line galaxies".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 19.9(2019):18.
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