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Searching for r-process-enhanced stars in the LAMOST surveyⅠ:the method
作者姓名:Tian-Yi Chen  Jian-Rong Shi  Timothy CBeers  Hong-Liang Yan  Qi Gao  Chun-Qian Li  Hai-Ning Li  Gang Zhao
作者单位:CAS Key Laboratory of Optical Astronomy;School of Astronomy and Space Science;Department of Physics and JINA Center for the Evolution of the Elements
基金项目:supported by National Key R&D Program of China(Grant No.2019YFA0405502);the Key Research Program of the Chinese Academy of Sciences(Grant No.XDPB09-02);the National Natural Science Foundation of China(Grant Nos.11833006,11473033,11603037,11973049,and 11973052);the international partnership program’s key foreign cooperation project,Bureau of International Cooperation,Chinese Academy of Sciences(Grant No.114A32KYSB20160049);the Strategic Priority Research Program of Chinese Academy of Sciences(Grant No.XDB34020205);supported by the Astronomical Big Data Joint Research Center,co-founded by the National Astronomical Observatories,Chinese Academy of Sciences and Alibaba Cloud;partial support for this work from grant PHY 14-30152;Physics Frontier Center/JINA Center for the Evolution of the Element(JINA-CEE),awarded by the US National Science Foundation;partially supported by the Open Project Program of the Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences;Funding for the project has been provided by the National Development and Reform Commission。
摘    要:The abundance patterns of r-process-enhanced stars contain key information required to constrain the astrophysical site(s)of r-process nucleosynthesis,and to deepen our understanding of the chemical evolution of our Galaxy.To expand the sample of known r-process-enhanced stars,we have developed a method to search for candidates in the LAMOST medium-resolution(R7500)spectroscopic survey by matching the observed spectra to synthetic templates around the EuⅡline at 6645.1 A.We obtain a sample of 13 metal-poor(-2.35
关 键 词:STARS  abundances-stars  chemically  peculiar-stars  STATISTICS
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