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Two New r-process-enhanced Stars with [Fe/H] >-0.6 dex from the LAMOST-MRS Survey
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作者 xiao-jin xie Jian-Rong Shi +8 位作者 Tian-Lu Chen Hong-Liang Yan Tian-Yi Chen Kai-Ke Pan Chun-Qian Li Shuai Liu Qi Gao Tai-Sheng Yan Ming-Yi Ding 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2022年第7期109-117,共9页
We report the discovery of two r-process-enhanced stars with [Fe/H]>-0.6 dex selected from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) survey.Three candidate stars have been selected from ... We report the discovery of two r-process-enhanced stars with [Fe/H]>-0.6 dex selected from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) survey.Three candidate stars have been selected from the LAMOST medium-resolution(R~ 7500) spectroscopic survey,and the follo wed-up high signal-to-noise ratio and high-resolution(R~31,500) spectra are obtained with the ARC Echelle Spectrograph mounted on the3.5 m telescope at the Apache Point Observatory,which allow us for the determination of stellar atmospheric parameters and abundances of 20 elements.Among these three r-process-enhanced candidate stars,TYC 1710-933-1 and TYC 2858-372-1 have [Eu/Fe] higher than 0.3 dex and [Ba/Eu] lower than 0.0 dex,thus,can be identified as new r-process-enhanced objects.TYC 2858-372-1 shows similar r+s-process pattern to the Sun.TYC 1710-933-1 presents enhancement of the r-process elements of Nd and Eu.Our work indicates that the enrichment mechanisms of the heavy neutron-capture elements are complicated for metal-rich stars. 展开更多
关键词 stars:abundances stars:chemically peculiar stars:fundamental parameters
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