基本信息
陈玉琴 女 博导 中国科学院国家天文台
电子邮件: cyq@nao.cas.cn
通信地址: 北京市朝阳区大屯路甲20号国家天文台A417
邮政编码: 100101
电子邮件: cyq@nao.cas.cn
通信地址: 北京市朝阳区大屯路甲20号国家天文台A417
邮政编码: 100101
研究领域
恒星光谱分析;
银河系化学演化
银河系化学演化
招生信息
招生专业
070401-天体物理
招生方向
元素丰度与星系化学演化
银河系恒星的化学和运动学参数确定
银河系恒星的化学和运动学参数确定
教育背景
学历
1990-1994 年: 北京师范大学天文学系
1994-2000年: 北京师范大学与北京天文台联合培养硕博连读研究生
1994-2000年: 北京师范大学与北京天文台联合培养硕博连读研究生
学位
博士
出国学习工作
1998-2000年: 丹麦奥尔胡斯大学物理与天文研究所 联合培养博士生
工作经历
工作简历
2000-2001 年: 国家天文台 助理研究员
2001-2005年: 国家天文台 副研究员
2005年-至今: 国家天文台 研究员
2008年: 国家天文台博士研究生指导教师
2001-2005年: 国家天文台 副研究员
2005年-至今: 国家天文台 研究员
2008年: 国家天文台博士研究生指导教师
专利与奖励
曾获得2003年度北京自然科学二等奖(排名第二)、2008年度国家自然科学二等奖(排名第二)和2009年度中国青年科技奖。
出版信息
发表论文
[1] Wu, Wenbo, Zhao, Gang, Chang, Jiang, Xue, XiangXiang, Chen, Yuqin, Li, Chengdong, Ye, Xianhao, Yang, Chengqun. Detection of Multiple Phase Space Overdensities of GSE Stars by Orbit Integration. ASTROPHYSICAL JOURNAL[J]. 2023, 950(2): http://dx.doi.org/10.3847/1538-4357/acd33a.[2] Yan, H H, Shi, W B, Chen, Y Q, Zhao, J K, Zhao, G. Evidence of a common origin for the Virgo overdensity and Hercules-Aquila Cloud from abundances and orbital parameters. ASTRONOMY & ASTROPHYSICS[J]. 2023, 674: http://dx.doi.org/10.1051/0004-6361/202346249.[3] Wu, Yaqian, Xiang, Maosheng, Zhao, Gang, Chen, Yuqin, Bi, Shaolan, Li, Yaguang. Timing the formation of the galactic thin disc with asteroseismic stellar ages. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2023, 520(2): 1913-1927, http://dx.doi.org/10.1093/mnras/stad223.[4] Jia, Yunpeng, Chen, Yuqin, Du, Cuihua, Zhao, Gang. Investigating the vertical distribution of the disk as a function of radial action. ASTRONOMY & ASTROPHYSICS[J]. 2023, 669: http://dx.doi.org/10.1051/0004-6361/202142977.[5] Fan, Zhou, Zhao, Gang, Wang, Wei, Zheng, Jie, Zhao, Jingkun, Li, Chun, Chen, Yuqin, Yuan, Haibo, Li, Haining, Tan, Kefeng, Song, Yihan, Zuo, Fang, Huang, Yang, Luo, Ali, Esamdin, Ali, Ma, Lu, Li, Bin, Song, Nan, Grupp, Frank, Zhao, Haibin, Ehgamberdiev, Shuhrat A, Burkhonov, Otabek A, Feng, Guojie, Bai, Chunhai, Zhang, Xuan, Niu, Hubiao, Khodjaev, Alisher S, Khafizov, Bakhodir M, Asfandiyarov, Ildar M, Shaymanov, Asadulla M, Karimov, Rivkat G, Yuldashev, Qudratillo, Lu, Hao, Zhaori, Getu, Hong, Renquan, Hu, Longfei, Liu, Yujuan, Xu, Zhijian. The Stellar Abundances and Galactic Evolution Survey (SAGES). I. General Description and the First Data Release (DR1). ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES[J]. 2023, 268(1): 18-, https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:001052545400001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=3a85505900f77cc629623c3f2907beab.[6] 陈玉琴. 基于LAMOST 数据的Sequoia 子结构研究. 天文学进展[J]. 2023, 41(3): [7] Xing, QianFan, Zhao, Gang, Liu, ZhengWei, Heger, Alexander, Han, ZhanWen, Aoki, Wako, Chen, YuQin, Ishigaki, Miho N, Li, HaiNing, Zhao, JingKun. A metal-poor star with abundances from a pair-instability supernova. NATURE[J]. 2023, 618(7966): 712-+, http://dx.doi.org/10.1038/s41586-023-06028-1.[8] Zhang, Z, Shi, W B, Chen, Y Q, Zhao, Gang, Carrell, K, Zhang, H P. The Substructures in the Anticenter Region of the Milky Way. THE ASTROPHYSICAL JOURNAL[J]. 2022, 933(2): 151-169, [9] Li, Zhuohan, Zhao, Gang, Chen, Yuqin, Liang, Xilong, Zhao, Jingkun. The stellar parameters and elemental abundances from low-resolution spectra I: 1.2 million giants from LAMOST DR8. 2022, http://arxiv.org/abs/2207.05294.[10] Chen, Yuqin, Zhao, Gang, Zhang, Haopeng. Evidence for Corotation Origin of Super-metal-rich Stars in LAMOST-Gaia: Multiple Ridges with a Similar Slope in the ϕ versus L z Plane. The Astrophysical Journal Letters[J]. 2022, 936(1): L7-L12, [11] He, XuJiang, Luo, ALi, Chen, YuQin. Identification, mass, and age of primary red clump stars from spectral features derived with the LAMOST DR7. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2022, 512(2): 1710-1721, http://dx.doi.org/10.1093/mnras/stac484.[12] Li, Zhuohan, Zhao, Gang, Chen, Yuqin, Liang, Xilong, Zhao, Jingkun. The stellar parameters and elemental abundances from low-resolution spectra - I. 1.2 million giants from LAMOST DR8. Monthly Notices of the Royal Astronomical Society[J]. 2022, 517(4): 4875-4891, [13] Chen, Xunzhou, Ge, Zhishuai, Chen, Yuqin, Bi, Shaolan, Yu, Jie, Yang, Wuming, Ferguson, Jason W, Wu, Yaqian, Li, Yaguang. Ages of Main-sequence Turnoff Stars from the GALAH Survey. ASTROPHYSICAL JOURNAL[J]. 2022, 929(2): http://dx.doi.org/10.3847/1538-4357/ac55a1.[14] Zhang, Haopeng, Chen, Yuqin, Zhao, Gang, Zhao, Jingkun, Liang, Xilong, Li, Haining, Wu, Yaqian, Luo, Ali, Wang, Rui. High-{\alpha}-Metal-Rich stars in the LAMOST-MRS survey and its connection with the galactic bulge. 2021, http://arxiv.org/abs/2102.05999.[15] Wu, Yaqian, Xiang, Maosheng, Chen, Yuqin, Zhao, Gang, Bi, Shaolan, Li, Chengdong, Li, Yaguang, Huang, Yang. Age-metallicity dependent stellar kinematics of the Milky Way disc from LAMOST and Gaia. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2021, 501(4): 4917-4934, http://dx.doi.org/10.1093/mnras/staa3949.[16] Zhang, Haopeng, Chen, Yuqin, Zhao, Gang. Radial Migration from the Metallicity Gradient of Open Clusters and Outliers. ASTROPHYSICAL JOURNAL[J]. 2021, 919(1): http://dx.doi.org/10.3847/1538-4357/ac0e92.[17] Gang Zhao, Yuqin Chen. Low-α metal-rich stars with sausage kinematics in the LAMOST survey: Are they from the Gaia-Sausage-Enceladus galaxy?. 中国科学:物理学、力学、天文学英文版[J]. 2021, 64(3): 14-26, http://lib.cqvip.com/Qikan/Article/Detail?id=7104079677.[18] Zhao, Gang, Chen, Yuqin. Low-alpha metal-rich stars with sausage kinematics in the LAMOST survey: Are they from the Gaia-Sausage-Enceladus galaxy?. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2021, 64(3): https://www.webofscience.com/wos/woscc/full-record/WOS:000616492700001.[19] Liang, XiLong, Chen, YuQin, Zhao, JingKun, Zhao, Gang. Partitioning the Galactic halo with Gaussian Mixture Models. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2021, 21(5): 274-286, http://dx.doi.org/10.1088/1674-4527/21/5/128.[20] Liang Xilong, Zhao Jingkun, Chen Yuqin, Fang Xiangsong, Ye Xianhao, Zhang Jiajun, Kong Xiaoming, Zhao Gang. A new moving group in the Local Arm. 2020, http://arxiv.org/abs/2003.05592.[21] Chen, Xunzhou, Ge, Zhishuai, Chen, Yuqin, Bi, Shaolan, Yu, Jie, Li, Tanda, Li, Yaguang, Ferguson, J W, Zhang, Jinghua, Wu, Yaqian. Ages of Dwarfs in the Solar Neighborhood: Considering C and O Enhancements. ASTROPHYSICAL JOURNAL[J]. 2020, 889(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000537752700002.[22] Chen, Y Q, Zhao, G. Open clusters as tracers on radial migration of the galactic disc. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2020, 495(3): 2673-2681, http://apps.webofknowledge.com/CitedFullRecord.do?product=UA&colName=WOS&SID=5CCFccWmJJRAuMzNPjj&search_mode=CitedFullRecord&isickref=WOS:000543025500013.[23] 曲大铭, 陈玉琴, 张浩鹏, 赵刚. 利用APOGEE的超富金属星研究银盘恒星的径向迁移效应. 天文研究与技术[J]. 2020, 17(3): 265-275, http://lib.cqvip.com/Qikan/Article/Detail?id=7102172344.[24] Liang, Xilong, Zhao, Jingkun, Chen, Yuqin, Fang, Xiangsong, Ye, Xianhao, Zhang, Jiajun, Kong, Xiaoming, Zhao, Gang. A New Moving Group in the Local Arm. ASTRONOMICAL JOURNAL[J]. 2020, 159(5): https://www.webofscience.com/wos/woscc/full-record/WOS:000525675200001.[25] Yan, Yepeng, Du, Cuihua, Liu, Shuai, Li, Hefan, Shi, Jianrong, Chen, Yuqin, Ma, Jun, Wu, Zhenyu. Chemical and Kinematic Properties of the Galactic Disk from the LAMOST and Gaia Sample Stars. ASTROPHYSICAL JOURNAL[J]. 2019, 880(1): http://dx.doi.org/10.3847/1538-4357/ab287d.[26] Du, Cuihua, Li, Hefan, Yan, Yepeng, Newberg, Heidi Jo, Shi, Jianrong, Ma, Jun, Chen, Yuqin, Wu, Zhenyu. New Nearby Hypervelocity Stars and Their Spatial Distribution from Gaia DR2. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES[J]. 2019, 244(1): https://www.webofscience.com/wos/woscc/full-record/WOS:000482572100002.[27] Liang, Xilong, Zhao, Jingkun, Chen, Yuqin, Zuo, Wenbo, Zhang, Jiajun, Zhu, Jia, Zhao, Gang. Elemental Abundance Distributions in the (R, V-phi) Plane with LAMOST DR5 and Gaia DR2. ASTROPHYSICAL JOURNAL[J]. 2019, 887(2): [28] Chen, Y Q, Zhao, G, Xue, X X, Zhao, J K, Liang, X L, Jia, Y P, Yang, C Q. A Hint of Three-section Halo As Seen from the APOGEE DR14. ASTROPHYSICAL JOURNAL[J]. 2019, 871(2): http://dx.doi.org/10.3847/1538-4357/aaf80f.[29] Chen, Y Q, Zhao, G, Zhao, J K, Liang, X L, Wu, Y Q, Jia, Y P, Tian, H, Liu, J M. Super Metal-rich Stars in the LAMOST Survey: A Test on Radial Migration. ASTRONOMICAL JOURNAL[J]. 2019, 158(6): https://www.webofscience.com/wos/woscc/full-record/WOS:000498859900001.[30] Jia, Yunpeng, Chen, Yuqin, Zhao, Gang, Xue, Xiangxiang, Zhao, Jingkun, Yang, Chengqun, Li, Chengdong. On the Radial Metallicity Gradient and Radial Migration Effect of the Galactic Disk. ASTROPHYSICAL JOURNAL[J]. 2018, 863(1): http://dx.doi.org/10.3847/1538-4357/aad3bb.[31] Zhao, Jingkun, Zhao, G, Aoki, W, Ishigaki, M N, Suda, T, Matsuno, T, Shi, J R, Xing, Q F, Chen, Y Q, Oswalt, Terry D, Kong, X M, Liang, X L. Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1. ASTROPHYSICAL JOURNAL[J]. 2018, 868(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000451432300018.[32] Liu, Shuai, Du, Cuihua, Newberg, Heidi Jo, Chen, Yuqin, Wu, Zhenyu, Ma, Jun, Zhou, Xu, Cao, Zihuang, Hou, Yonghui, Wang, Yuefei, Zhang, Yong. Metallicity and Kinematics of the Galactic Halo from the LAMOST Sample Stars. ASTROPHYSICAL JOURNAL[J]. 2018, 862(2): http://dx.doi.org/10.3847/1538-4357/aacf91.[33] Du, Cuihua, Li, Hefan, Newberg, Heidi Jo, Chen, Yuqin, Shi, Jianrong, Wu, Zhenyu, Ma, Jun. The Origin of High-velocity Stars from Gaia and LAMOST. ASTROPHYSICAL JOURNAL LETTERS[J]. 2018, 869(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000453856800001.[34] Liang, X L, Zhao, J K, Zhao, G, Aoki, W, Ishigaki, M N, Matsuno, T, Chen, Y Q, Kong, X M, Shi, J R, Xing, Q F. Tracing the Origin of Moving Groups. I. The ? Leo Moving Group with High-resolution Spectra from the Subaru Telescope. ASTROPHYSICAL JOURNAL[J]. 2018, 863(1): http://dx.doi.org/10.3847/1538-4357/aacf8a.[35] Wang, Wei, Wang, Liang, Li, Xiang, Chen, Yuqin, Zhao, Gang. Giant Planets around FGK Stars Probably Form through Core Accretion. ASTROPHYSICALJOURNAL[J]. 2018, 860(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000435935300013.[36] Jia, Y P, Chen, Y Q, Zhao, G, Bari, M A, Zhao, J K, Tan, K F. Abundance patterns of evolved stars with Hipparcos parallaxes and ages based on the APOGEE data base. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2018, 473(2): 2622-2632, http://dx.doi.org/10.1093/mnras/stx2504.[37] Zhang, X, Shi, W B, Chen, Y Q, Zhao, G, Carrell, K, Zhao, J K, Ruan, G P, Liang, Y C, Zhou, L, Ren, H B, Zhang, Y, Hou, Y H, Wang, Y F. The properties of red giant stars along the Sagittarius tidal tails. ASTRONOMY & ASTROPHYSICS[J]. 2017, 597: http://ir.bao.ac.cn/handle/114a11/8267.[38] 梁熙龙, 赵景昆, 陈玉琴, 赵刚. 太阳邻域晕流的研究进展. 天文学进展[J]. 2017, 35(2): 175-, http://lib.cqvip.com/Qikan/Article/Detail?id=672352578.[39] Liang, X L, Zhao, J K, Oswalt, T D, Chen, Y Q, Zhang, L, Zhao, G. Stellar Stream Candidates in the Solar Neighborhood Found in the LAMOST DR3 and TGAS. ASTROPHYSICAL JOURNAL[J]. 2017, 844(2): http://ir.bao.ac.cn/handle/114a11/20068.[40] Chen, Y Q, Casagrande, L, Zhao, G, Bovy, J, Aguirre, V Silva, Zhao, J K, Jia, Y P. Absolute Magnitudes of Seismic Red Clumps in the Kepler Field and SAGA: The Age Dependency of the Distance Scale. ASTROPHYSICAL JOURNAL[J]. 2017, 840(2): http://dx.doi.org/10.3847/1538-4357/aa6d0f.[41] Takeda, Y, Tajitsu, A, Sato, B, Liu, Y J, Chen, Y Q, Zhao, G. Fundamental stellar parameters and age-metallicity relation of Kepler red giants in comparison with theoretical evolutionary tracks. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2016, 457(4): 4454-4469, https://www.webofscience.com/wos/woscc/full-record/WOS:000373586000077.[42] Jing, Yingjie, Du, Cuihua, Gu, Jiayin, Jia, Yunpeng, Peng, Xiyan, Chen, Yuqin, Wu, Zhenyu, Ma, Jun, Zhou, Xu, Cao, Zihuang, Hou, Yonghui, Wang, Yuefei, Zhang, Yong. Kinematics of the Galactic disc from a LAMOST dwarf sample. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2016, 463(3): 3390-3397, http://dx.doi.org/10.1093/mnras/stw2230.[43] 陈玉琴. AGES OF 70 DWARFS OF THREE POPULATIONS IN THE SOLAR NEIGHBORHOOD: CONSIDERING O AND C ABUNDANCES IN STELLAR MODEL. ApJ, 833, 161. 2016, [44] GuoChao Yang, YanChun Liang, YuQin Chen, Gang Zhao, Bo Zhang, GuoQing Liu, YuJuan Liu, Nian Liu, LiCai Deng, CaiXia Zhang. Chemical abundance analysis of 19 barium stars. 天文和天体物理学研究(英文版). 2016, [45] Yang, GuoChao, Liang, YanChun, Spite, Monique, Chen, YuQin, Zhao, Gang, Zhang, Bo, Liu, GuoQing, Liu, YuJuan, Liu, Nian, Deng, LiCai, Spite, Francois, Hill, Vanessa, Zhang, CaiXia. Chemical abundance analysis of 19 barium stars. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2016, 16(1): http://ir.bao.ac.cn/handle/114a11/5466.[46] Fang, XiangSong, Zhao, Gang, Zhao, JingKun, Chen, YuQin, Kumar, Yerra Bharat. Stellar activity with LAMOST - I. Spot configuration in Pleiades. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2016, 463(3): 2494-2512, http://ir.bao.ac.cn/handle/114a11/8300.[47] 陈玉琴. Chemical abundances of member stars in the open cluster NGC2632. 2015, AJ< 150, 158. 2015, [48] 李响, 赵刚, 陈玉琴. mg超丰恒星的性质及其起源的研究. 天文研究与技术[J]. 2015, 12(2): 127-, [49] Chen, YuQin, Zhao, Gang, Liu, Chao, Ren, Jing, Jia, YunPeng, Zhao, JingKun, Luo, ALi, Wu, Yue, Zhang, Yong, Hou, YongHui, Wang, YueFei, Yang, Ming. A comparison of stellar atmospheric parameters from the LAMOST and APOGEE datasets. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2015, 15(8): 1125-1136, http://sciencechina.cn/gw.jsp?action=detail.jsp&internal_id=5501532&detailType=1.[50] Zhao Jingkun, Oswalt Terry D, Chen Yuqin, Shi Jianrong, Tan Kefeng, Fang Xiangsong, Zhao Gang, Yang Ming, Zhang Yong, Hou Yonghui, Wang Yuefei. caiihkemissiondistributionof120000fgandkstarsinlamostdr1. RESEARCHINASTRONOMYANDASTROPHYSICS[J]. 2015, 15(8): 1282-, [51] Zhao, JingKun, Zhao, Gang, Chen, YuQin, Tan, KeFeng, Gao, MengTian, Yang, Ming, Zhang, Yong, Hou, YongHui. Halo stream candidates in the LAMOST DR2. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2015, 15(8): 1378-1391, http://ir.bao.ac.cn/handle/114a11/5602.[52] Yang XiaoLing, Chen YuQin, Zhao Gang. Planet host stars in open clusters. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2015, 58(3): http://ir.bao.ac.cn/handle/114a11/6650.[53] Zhao, JingKun, Oswalt, Terry D, Chen, YuQin, Shi, JianRong, Tan, KeFeng, Fang, XiangSong, Zhao, Gang, Yang, Ming, Zhang, Yong, Hou, YongHui, Wang, YueFei. CaII H&K emission distribution of similar to 120 000 F, G and K stars in LAMOST DR1. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2015, 15(8): 1282-1293, http://ir.bao.ac.cn/handle/114a11/5610.[54] Li, Xiang, Zhao, Gang, Chen, YuQin, Li, HaiNing. A search for strongly Mg-enhanced stars from the Sloan Digital Sky Survey. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2014, 14(11): 1423-1437, http://ir.bao.ac.cn/handle/114a11/6521.[55] Tan, Kefeng, Chen, Yuqin, Carrell, Kenneth, Zhao, Jingkun, Zhao, Gang. RED GIANT STARS FROM THE SLOAN DIGITAL SKY SURVEY. II. DISTANCES. ASTROPHYSICAL JOURNAL[J]. 2014, 794(1): http://ir.bao.ac.cn/handle/114a11/6529.[56] Nissen, P E, Chen, Y Q, Carigi, L, Schuster, W J, Zhao, G. Carbon and oxygen abundances in stellar populations. ASTRONOMY & ASTROPHYSICS[J]. 2014, 568: http://ir.bao.ac.cn/handle/114a11/6434.[57] Chen, Y Q, Zhao, G, Carrell, K, Zhao, J K, Tan, K F, Nissen, P E, Wei, P. RED GIANT STARS FROM SLOAN DIGITAL SKY SURVEY. I. THE GENERAL FIELD. ASTROPHYSICAL JOURNAL[J]. 2014, 795(1): http://dx.doi.org/10.1088/0004-637X/795/1/52.[58] Zhao, Jingkun, Zhao, G, Chen, Y Q, Oswalt, T D, Tan, K F, Zhang, Y. THREE MOVING GROUPS DETECTED IN THE LAMOST DR1 ARCHIVE. ASTROPHYSICAL JOURNAL[J]. 2014, 787(1): http://ir.bao.ac.cn/handle/114a11/6402.[59] 陈玉琴. RED GIANT STARS FROM SLOAN DIGITAL SKY SURVEY II. DISTANCE. 2014, APJ, 794, 60. 2014, [60] Chen, Y Q, Zhao, G, Carrell, K, Zhao, J K, Tan, K F. THE CH(G) INDEX AS A NEW CRITERION FOR SELECTING RED GIANT STARS. ASTROPHYSICAL JOURNAL[J]. 2013, 765(2): http://dx.doi.org/10.1088/0004-637X/765/2/156.[61] Liu, Shu, Zhao, Gang, Chen, YuQin, Takeda, Yoichi, Honda, Satoshi. Abundances of 23 field RR Lyrae stars. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2013, 13(11): 1307-1329, http://ir.bao.ac.cn/handle/114a11/5831.[62] Chen, Li, Hou, JinLiang, Yu, JinCheng, Liu, Chao, Deng, LiCai, Newberg, Heidi Jo, Carlin, Jeffrey L, Yang, Fan, Zhang, YueYang, Shen, ShiYin, Zhang, HaoTong, Chen, JianJun, Chen, YuQin, Christlieb, Norbert, Han, ZhanWen, Lee, HsuTai, Liu, XiaoWei, Pan, KaiKe, Shi, JianRong, Wang, HongChi, Zhu, Zi. The LEGUE disk targets for LAMOST's pilot survey. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2012, 12(7): 805-812, http://lib.cqvip.com/Qikan/Article/Detail?id=42665206.[63] Carlin, Jeffrey L, Lepine, Sebastien, Newberg, Heidi Jo, Deng, LiCai, Beers, Timothy C, Chen, YuQin, Christlieb, Norbert, Fu, XiaoTing, Gao, Shuang, Grillmair, Carl J, Guhathakurta, Puragra, Han, ZhanWen, Hou, JinLiang, Lee, HsuTai, Li, Jing, Liu, Chao, Liu, XiaoWei, Pan, KaiKe, Sellwood, J A, Wang, HongChi, Yang, Fan, Yanny, Brian, Zhang, YueYang, Zheng, Zheng, Zhu, Zi. An algorithm for preferential selection of spectroscopic targets in LEGUE. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2012, 12(7): 755-771, http://lib.cqvip.com/Qikan/Article/Detail?id=42665202.[64] Carrell, Kenneth, Chen, Yuqin, Zhao, Gang. METALLICITY GRADIENTS OF THICK DISK DWARF STARS. ASTRONOMICAL JOURNAL[J]. 2012, 144(6): http://dx.doi.org/10.1088/0004-6256/144/6/185.[65] Shi, W B, Chen, Y Q, Carrell, K, Zhao, G. THE KINEMATICS AND CHEMISTRY OF RED HORIZONTAL BRANCH STARS IN THE SAGITTARIUS STREAMS. ASTROPHYSICAL JOURNAL[J]. 2012, 751(2): http://ir.bao.ac.cn/handle/114a11/6279.[66] Carrell, Kenneth, Wilhelm, Ronald, Chen, YuQin. RED CLUMP STARS IN THE SAGITTARIUS TIDAL STREAMS. ASTRONOMICAL JOURNAL[J]. 2012, 144(1): http://dx.doi.org/10.1088/0004-6256/144/1/18.[67] Deng, LiCai, Newberg, Heidi Jo, Liu, Chao, Carlin, Jeffrey L, Beers, Timothy C, Chen, Li, Chen, YuQin, Christlieb, Norbert, Grillmair, Carl J, Guhathakurta, Puragra, Han, ZhanWen, Hou, JinLiang, Lee, HsuTai, Lepine, Sebastien, Li, Jing, Liu, XiaoWei, Pan, KaiKe, Sellwood, J A, Wang, Bo, Wang, HongChi, Yang, Fan, Yanny, Brian, Zhang, HaoTong, Zhang, YueYang, Zheng, Zheng, Zhu, Zi. LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) - The survey's science plan. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2012, 12(7): 735-754, http://lib.cqvip.com/Qikan/Article/Detail?id=42665201.[68] Liu, F, Chen, Y Q, Zhao, G, Han, I, Lee, B C, Kim, K M, Zhao, Z S. Chemical composition of giants from two moving groups. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2012, 422(4): 2969-2979, http://ir.bao.ac.cn/handle/114a11/6123.[69] Jing-KunZhao GangZhao Yu-QinChen A-LiLuo. Metallicity calibration for solar type stars based on red spectra. 天文和天体物理学研究:英文版[J]. 2011, 11(5): 563-576, http://lib.cqvip.com/Qikan/Article/Detail?id=37982215.[70] Zhao, JingKun, Zhao, Gang, Chen, YuQin, Luo, ALi. Metallicity calibration for solar type stars based on red spectra. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2011, 11(5): 563-576, http://lib.cqvip.com/Qikan/Article/Detail?id=37982215.[71] 陈玉琴. Spectroscopic study of two solar twin candidates and the colors of the Sun. Science in China Series G:Physics,Mechanics and Astronomy, 53 ,579,2010. 2010, [72] Chen, Y Q, Zhao, G, Zhao, J K, Xue, X X, Schuster, W J. METALLICITY AND KINEMATIC DISTRIBUTIONS OF RED HORIZONTAL-BRANCH STARS FROM THE SDSS SURVEY. ASTRONOMICAL JOURNAL[J]. 2010, 140(2): 500-509, http://ir.bao.ac.cn/handle/114a11/7781.[73] Zhao ZhengShi, Chen YuQin, Zhao JingKun, Zhao Gang. Spectral analysis of two solar twins and the colors of the Sun. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2010, 53(3): 579-585, http://dx.doi.org/10.1007/s11433-009-0228-5.[74] Zhao, Jingkun, Zhao, Gang, Chen, Yuqin. A CATALOG OF MOVING GROUP CANDIDATES IN THE SOLAR NEIGHBORHOOD. ASTROPHYSICAL JOURNAL LETTERS[J]. 2009, 692(2): L113-L117, http://dx.doi.org/10.1088/0004-637X/692/2/L113.[75] 陈玉琴. The abosolute magnitude of red horizontal branch stars in the ugriz system. 2009, ApJ, 702,1336. 2009, [76] 赵正实, 陈玉琴, 赵景昆, 赵刚. 两颗太阳孪生星的光谱分析与太阳颜色的确定. 中国科学G辑物理学力学天文学[J]. 2009, 1161-, http://lib.cqvip.com/Qikan/Article/Detail?id=31313289.[77] 赵正实, 陈玉琴, 赵景昆, 赵刚. 两颗太阳孪生星的光谱分析与太阳颜色的确定. 中国科学:G辑[J]. 2009, 1161-1168, http://lib.cqvip.com/Qikan/Article/Detail?id=31313289.[78] Chen, Y Q, Zhao, G, Izumiura, H, Zhao, J K, Liu, Y J, Honda, S, Ohkubo, M. Abundance pattern of metal-rich stars from 14 old and 24 young stars. ASTRONOMICAL JOURNAL[J]. 2008, 135(2): 618-630, http://ir.bao.ac.cn/handle/114a11/7341.[79] 赵景昆, 赵刚, 陈玉琴. 高分辨率恒星光谱处理与元素丰度分析软件平台. 天文研究与技术:国家天文台台刊[J]. 2007, 4(2): 153-158, http://lib.cqvip.com/Qikan/Article/Detail?id=24745267.[80] 赵景昆, 赵刚, 陈玉琴. 高分辨率恒星光谱处理与元素丰度分析软件平台. 天文研究与技术[J]. 2007, 4(2): 153-, http://lib.cqvip.com/Qikan/Article/Detail?id=24745267.[81] Zhao, JingKun, Zhao, Gang, Chen, YuQin, Shi, JianRong, Liu, YuJuan, Zhang, JuYong. Automatic normalization and equivalent-width measurement of high-resolution stellar spectra. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS[J]. 2006, 6(6): 689-696, http://ir.bao.ac.cn/handle/114a11/7070.[82] 崔辰州, 陈玉琴, 赵刚, 赵永恒. 银盘恒星的金属丰度梯度. 中国科学:A辑[J]. 2002, 32(8): 761-768, http://lib.cqvip.com/Qikan/Article/Detail?id=6649713.[83] Qiu Hongmei, Chen Yuqin, Zhao Gang. Equivalent Widthe os 15 Extrasolar—Planet Host Stars. 中国天文和天体物理学报:英文版[J]. 2002, 2(4): 377-390, http://lib.cqvip.com/Qikan/Article/Detail?id=6710938.[84] 崔辰州, 陈玉琴. 银盘恒星的金属丰度梯度. 中国科学A辑数学[J]. 2002, 32(8): 761-, http://lib.cqvip.com/Qikan/Article/Detail?id=6649713.[85] 赵刚, 李宗伟, 唐仕奎, 陈玉琴, 邱红梅. 有行星系统恒星的金属丰度研究. 北京师范大学学报:自然科学版[J]. 2001, 37(1): 31-, http://lib.cqvip.com/Qikan/Article/Detail?id=4973781.[86] Chen, Y. Q., Zhao, G., Liu, C., Ren, J., Jia, Y. P., Zhao, J. K., Luo, A. L., Zhang, Y., Hou, Y. H., Wang, Y. F., Yang, M.. 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科研活动
科研项目
独立主持了:
国家自然科学基金委学部主任专项基金
青年科学基金(具有行星系统恒星的化学丰度星研究)
面上项目(SDSS晚型恒星数据的系统分析)
目前正在研究:
面上项目(银河系矮星和巨星的丰度分析)
作为课题骨干人员,参加:
国家自然科学基金重点项目“银河系结构与演化”
中国科学院知识创新工程重要方向性项目“大样本恒星观测与理论研究及其在银河系与宇宙学研究中的应用”(并担任子课题负责人)
国家自然科学基金群体创新项目“星系结构与黑洞”
国家科技部973项目“星系形成与演化”
国家自然科学基金委学部主任专项基金
青年科学基金(具有行星系统恒星的化学丰度星研究)
面上项目(SDSS晚型恒星数据的系统分析)
目前正在研究:
面上项目(银河系矮星和巨星的丰度分析)
作为课题骨干人员,参加:
国家自然科学基金重点项目“银河系结构与演化”
中国科学院知识创新工程重要方向性项目“大样本恒星观测与理论研究及其在银河系与宇宙学研究中的应用”(并担任子课题负责人)
国家自然科学基金群体创新项目“星系结构与黑洞”
国家科技部973项目“星系形成与演化”
指导学生
已指导学生
赵正实 硕士研究生 070401-天体物理
现指导学生
狄龙 博士研究生 070401-天体物理