发表论文
[1] QianSheng Zhang, Yan Li, Tao Wu, Chen Jiang. Asteroseismic Investigation on KIC 10526294 to Probe Convective Core Overshoot Mixing. THE ASTROPHYSICAL JOURNAL[J]. 2023, 953(1): https://doaj.org/article/9cc173c9a8cc467989984a0e4e7ec8d5.[2] Song, Fen, Yuan, Zunli, Li, Yan, Wu, Xuchao, Pietrinferni, Adriano, Poon, Helen, Wu, Tao, Nie, Jundan, Song, Hanfeng, Han, Cheng, Yang, Ye, Li, Yuxuan, Bai, Xingming. Red giant branch bump brightness in 7 metal-poor globular clusters obtained with GAIA DR2. ASTROPHYSICS AND SPACE SCIENCE[J]. 2022, 367(3): [3] Zhang, QianSheng, ChristensenDalsgaard, Jorgen, Li, Yan. Core overshoot constrained by the absence of a solar convective core and some solar-like stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2022, 512(4): 4852-4868, http://dx.doi.org/10.1093/mnras/stac766.[4] Guo, Fei, Li, Yan. Convective Overshooting in the Envelopes of A-type Stars Using the k-omega Model. ASTROPHYSICAL JOURNAL[J]. 2021, 910(1): https://www.webofscience.com/wos/woscc/full-record/WOS:000632371000001.[5] Yan, HongLiang, Zhou, YuTao, Zhang, Xianfei, Li, Yaguang, Gao, Qi, Shi, JianRong, Zhao, Gang, Aoki, Wako, Matsuno, Tadafumi, Li, Yan, Xu, XiaoDong, Li, Haining, Wu, YaQian, Jin, MengQi, Mosser, Benoit, Bi, ShaoLan, Fu, JianNing, Pan, Kaike, Suda, Takuma, Liu, YuJuan, Zhao, JingKun, Liang, XiLong. Most lithium-rich low-mass evolved stars revealed as red clump stars by asteroseismology and spectroscopy. NATURE ASTRONOMY[J]. 2021, 5(1): https://www.webofscience.com/wos/woscc/full-record/WOS:000575344500001.[6] 李焱. 小尺度磁场是否是造成太阳p模式震荡表面效应的主要原因. Astrophysical Journal[J]. 2021, [7] Li, Yan, Zhang, Qiansheng, Wu, Tao, Su, Jie, Chen, Xinghao, Lin, Guifang, Guo, Jianheng, Liu, Jieying. Can Small-scale Magnetic Fields Be the Major Cause for the Near-surface Effect of the Solar p-mode Frequencies?. ASTROPHYSICAL JOURNAL[J]. 2021, 916(2): [8] Chen, Xinghao, Zhang, Xiaobin, Li, Yan, Chen, Hailiang, Luo, Changqing, Su, Jie, Chen, Xuefei, Han, Zhanwen. KIC 10736223: An Algol-type Eclipsing Binary That Has Just Undergone the Rapid Mass-transfer Stage. ASTROPHYSICAL JOURNAL[J]. 2020, 895(2): http://dx.doi.org/10.3847/1538-4357/ab8bd2.[9] Zhang, Xinyi, Li, Yan, Wu, Tao, Su, Jie. Determining the size of the helium core of KIC 9970396 using asteroseismology: a red giant approaching the red giant bump. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2020, 494(1): 511-528, http://dx.doi.org/10.1093/mnras/staa667.[10] Wu, Tao, Li, Yan, Deng, Zhenmin, Lin, Guifang, Song, Hanfeng, Jiang, Chen. Asteroseismic Analyses of Slowly Pulsating B Star KIC 8324482: Ultraweak Element Mixing beyond the Central Convective Core. ASTROPHYSICAL JOURNAL[J]. 2020, 899(1): http://dx.doi.org/10.3847/1538-4357/aba430.[11] 李焱. 慢脉动B型星KIC 8324482的星震学分析: 中央对流核外的极弱元素混合. Astrophysical Journal. 2020, [12] 李焱. KIC 10736223: 一颗刚刚经历快速物质转移阶段的Algol型双星. Astrophysical Journal. 2020, [13] Zhang, Xiaobin, Chen, Xinghao, Zhang, Haotong, Fu, Jianning, Li, Yan. A Pre-main-sequence gamma Dor-delta Sct Hybrid with Extremely Slow Internal Rotation in a Short-period Eclipsing Binary KIC 9850387 Revealed by Asteroseismology. ASTROPHYSICAL JOURNAL[J]. 2020, 895(2): http://dx.doi.org/10.3847/1538-4357/ab8ad5.[14] 李焱. 用星震学确定KIC 9970396的氦核大小:一颗接近红巨星bump的恒星. MNRAS. 2020, [15] 张孝斌, Chen Xinghao, Fu, JianNing, Li Yan. A Pre-main-sequence γ Dor-δ Sct Hybrid with Extremely Slow Internal Rotation in a Short-period Eclipsing Binary KIC 9850387 Revealed by Asteroseismology. The Astrophysical Journal[J]. 2020, 895(2): 124, [16] 李焱. 一颗主序前盾牌座δ型变星IP Per的星震学. Astrophysical Journal. 2019, [17] Li, Yan, Chen, Xinghao, Chen, Hailiang. Overshooting in the Core Helium-burning Stage of a 30M(circle dot) Star Using the k-omega Model. ASTROPHYSICAL JOURNAL[J]. 2019, 870(2): http://ir.ynao.ac.cn/handle/114a53/18956.[18] 李焱. 利用k-ω模型研究低质量恒星的对流超射. Astrophysical Journal. 2019, [19] 李焱. 星震学进展. 2019, [20] 李焱. 利用k-omega模型研究一颗30太阳质量恒星氦燃烧期间对流超射过程. Astrophysical Journal[J]. 2019, [21] Zhang, QianSheng, Li, Yan, ChristensenDalsgaard, Jorgen. Solar Models with Convective Overshoot, Solar-wind Mass Loss, and PMS Disk Accretion: Helioseismic Quantities, Li Depletion, and Neutrino Fluxes. ASTROPHYSICAL JOURNAL[J]. 2019, 881(2): http://dx.doi.org/10.3847/1538-4357/ab2f77.[22] 李焱. 具有对流超射、太阳风物质损失和盘吸积的太阳模型:日震学量、锂耗散和中微子. Astrophysical Journal. 2019, [23] Chen, Xinghao, Li, Yan, Zhang, Xiaobin. Exploring the Convective Core of the Hybrid delta Scuti-gamma Doradus Star CoRoT 100866999 with Asteroseismology. ASTROPHYSICALJOURNAL[J]. 2019, 887(2): http://dx.doi.org/10.3847/1538-4357/ab585b.[24] 李焱. 慢脉动B型星HD 50230的高精度星震学. Astrophysical Journal. 2019, [25] Chen, Xinghao, Li, Yan. Asteroseismology of the Pre-main-sequence delta Scuti Pulsator IP Persei. ASTROPHYSICAL JOURNAL[J]. 2019, 872(2): http://ir.ynao.ac.cn/handle/114a53/19366.[26] Guo, Fei, Li, Yan. Convective Overshooting in Low-mass Stars Using the k-omega Model. ASTROPHYSICAL JOURNAL[J]. 2019, 879(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000474921300002.[27] Wu, Tao, Li, Yan. High-precision Asteroseismology in a Slowly Pulsating B Star: HD 50230. ASTROPHYSICAL JOURNAL[J]. 2019, 881(1): https://www.webofscience.com/wos/woscc/full-record/WOS:000481848600015.[28] 李焱. 用星震学探索δ Scuti-γ Doradus型恒星CoRoT 100866999的对流核. Astrophysical Journal. 2019, [29] 陈雪飞, 李焱, 韩占文. 双致密星引力波源的形成. 中国科学物理学力学天文学[J]. 2018, 48(7): 079803, http://lib.cqvip.com/Qikan/Article/Detail?id=675611515.[30] Li, Yan, Chen, Xinghao, Xiong, Heran, Guo, Junjun, Chen, Xuefei, Han, Zhanwen. Convective Overshooting in sdB Stars Using the k-omega Model. ASTROPHYSICAL JOURNAL[J]. 2018, 863(1): http://dx.doi.org/10.3847/1538-4357/aacdf9.[31] Zhang, Xinyi, Wu, Tao, Li, Yan. Frequency Identification and Asteroseismic Analysis of the Red Giant KIC 9145955: Fundamental Parameters and Helium Core Size. ASTROPHYSICAL JOURNAL[J]. 2018, 855(1): https://www.webofscience.com/wos/woscc/full-record/WOS:000426374700009.[32] Wu, Tao, Li, Yan. Which evolutionary status does the Blue Large-Amplitude Pulsators stay at?. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2018, 478(3): 3871-3877, http://dx.doi.org/10.1093/mnras/sty1347.[33] Chen, Xinghao, Li, Yan. Determining the Evolutionary Stage of the delta Scuti Star HIP 80088 with Asteroseismology. ASTROPHYSICAL JOURNAL[J]. 2018, 866(2): http://ir.ynao.ac.cn/handle/114a53/18016.[34] Nikolay N. Samus, Yan Li. Preface: Stars and interstellar medium. 天文和天体物理学研究:英文版[J]. 2018, 18(8): 1-3, http://lib.cqvip.com/Qikan/Article/Detail?id=676043901.[35] Samus, Nikolay N, Li, Yan. Preface: Stars and interstellar medium. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2018, 18(8): http://lib.cqvip.com/Qikan/Article/Detail?id=676043901.[36] 邓真敏, 李焱, 吴涛, 陈兴浩. 慢脉动B型星KIC 8324482的星震学研究. 天文学报[J]. 2018, 59(5): 49, http://lib.cqvip.com/Qikan/Article/Detail?id=7000843705.[37] Song, Fen, Li, Yan, Wu, Tao, Pietrinferni, Adriano, Poon, Helen, Xie, Yi. The Influence of the Metal Mass Fraction Z, Age, and Mixing-length Parameter on the RGB Bump Magnitude for the M4 Cluster. ASTROPHYSICAL JOURNAL[J]. 2018, 869(2): http://ir.ynao.ac.cn/handle/114a53/18602.[38] Wu, Tao, Li, Yan, Deng, Zhenmin. A New C-D-like Diagram for SPB Stars: The Variations of Period Spacing as a Signature of Evolutionary Status. ASTROPHYSICAL JOURNAL[J]. 2018, 867(1): http://ir.ynao.ac.cn/handle/114a53/18319.[39] Chen XueFei, Li Yan, Han ZhanWen. The formation of double compact objects as gravitational wave sources. SCIENTIA SINICA-PHYSICA MECHANICA & ASTRONOMICA[J]. 2018, 48(7): [40] Guo, JunJun, Li, Yan. Influence of the He-flash convective overshoot on mode trapping efficiency in g-mode pulsating subdwarf B stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2018, 478(3): 3290-3297, http://dx.doi.org/10.1093/mnras/sty1010.[41] 李焱. 采用k-omega模型处理sdB恒星中的对流超射. ApJ. 2018, [42] Chen, Xinghao, Li, Yan. Rotational Splitting and Asteroseismic Modeling of the delta Scuti Star EE Camelopardalis. ASTROPHYSICAL JOURNAL[J]. 2017, 838(1): http://ir.ynao.ac.cn/handle/114a53/9984.[43] Wu Tao, Li Yan, Monteiro MJPFG, Cunha MS, Ferreira JMTS. New Insights of High-precision Asteroseismology: Acoustic Radius and chi(2)-matching Method for Solar-like Oscillator KIC 6225718. SEISMOLOGY OF THE SUN AND THE DISTANT STARS 2016-USING TODAY'S SUCCESSES TO PREPARE THE FUTURE[J]. 2017, 160: [44] Niu, JiaShu, Fu, JianNing, Li, Yan, Yang, XiaoHu, Zong, Weikai, Xue, HuiFang, Zhang, YanPing, Liu, Nian, Du, Bing, Zuo, Fang. AE Ursae Majoris - a delta Scuti star in the Hertzsprung Gap. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2017, 467(3): 3122-3139, http://ir.ynao.ac.cn/handle/114a53/10017.[45] Li, Yan. Applications of the k-omega Model in Stellar Evolutionary Models. ASTROPHYSICAL JOURNAL[J]. 2017, 841(1): http://dx.doi.org/10.3847/1538-4357/aa6d4e.[46] Wu, Tao, Li, Yan. An Independent Asteroseismic Analysis of the Fundamental Parameters and Internal Structure of the Solar-like Oscillator KIC 6225718. ASTROPHYSICAL JOURNAL[J]. 2017, 846(1): https://www.webofscience.com/wos/woscc/full-record/WOS:000408746000005.[47] Chen, Xinghao, Li, Yan, Lin, Guifang, Chen, Yanhui, Guo, Junjun. EXPLORING THE HELIUM CORE OF THE delta SCUTI STAR COROT 102749568 WITH ASTEROSEISMOLOGY. ASTROPHYSICAL JOURNAL[J]. 2017, 834(2): http://dx.doi.org/10.3847/1538-4357/834/2/146.[48] 李焱, Wu T Chinese Acad Sci Yunnan Observ POB Kunming Yunnan Peoples R China, 吴涛. New Insights of High-precision Asteroseismology: Acoustic Radius and chi(2)-matching Method for Solar-like Oscillator KIC 6225718. EPJWEBOFCONFERENCESSEISMOLOGYOFTHESUNANDTHEDISTANTSTARS2016USINGTODAYSSUCCESSESTOPREPARETHEFUTURE. 2017, 160: 1-4, [49] Fu, JN, Vauclair, G, Su, J, Cang, T, Li, C, Xue, H, Jiang, XJ, 李焱, Niu, H, Zhang, X, Colas, F, Dolez, N, Machado, LF, Michel, R, Alvarez, M, Kim, SL. Asteroseismology of the ZZ Ceti and DAZ GD 133. ASTRONOMICAL SOCIETY OF THE PACIFIC (ASP) CONFERENCE SERIES - 20TH EUROPEAN WHITE DWARF WORKSHOP. 2017, 509: 355-358, http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000401592100059&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=3a85505900f77cc629623c3f2907beab.[50] Wu, Tao, Li, Yan. NEW INSIGHTS FOR HIGH-PRECISION ASTEROSEISMOLOGY: ACOUSTIC RADIUS OF KIC 6225718. ASTROPHYSICAL JOURNAL LETTERS[J]. 2016, 818(1): http://www.irgrid.ac.cn/handle/1471x/1060402.[51] 郭志亮, 李焱. 恒星对流k—ω模型的性质研究. 天文学报[J]. 2014, 55(1): 66-77, http://lib.cqvip.com/Qikan/Article/Detail?id=48436813.[52] 郭志亮, 李焱. 恒星对流kw模型的性质研究. 天文学报[J]. 2014, 55(1): 66, [53] 郭志亮, 李焱. 恒星对流κ-ω模型的性质研究. 天文学报[J]. 2014, 55(1): 66-77, http://www.irgrid.ac.cn/handle/1471x/1049694.[54] Ding, CaiYun, Li, Yan. The influences of convective overshooting and semiconvection on the chemical evolution of massive stars. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2014, 14(8): 979-991, http://www.irgrid.ac.cn/handle/1471x/1049608.[55] Chen, YanHui, Li, Yan. Asteroseismology of DAV white dwarf stars and G29-38. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2013, 13(12): 1438-1444, http://www.irgrid.ac.cn/handle/1471x/1049599.[56] 李焱. 恒星对流的k-omega模型. 2013中国天文学会学术年会文集. 2013, 45, http://www.irgrid.ac.cn/handle/1471x/1008054.[57] 张瑞玉, 李焱. 存在非同步转动的双星演化模型. 天文学报[J]. 2012, 53(4): 274, http://lib.cqvip.com/Qikan/Article/Detail?id=42819958.[58] 李焱. 恒星湍热对流的k-omega模型. ApJ. 2012, [59] Guo, JunJun, Li, Yan, Lai, XiangJun. Avoided crossings between non-radial modes in low mass RGB stars. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2012, 12(12): 1655-1665, http://lib.cqvip.com/Qikan/Article/Detail?id=44238649.[60] Lai, XiangJun, Li, Yan. Chemical mixing by turbulent convection in the overshooting region below the convective envelope of RGB stars. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2011, 11(11): 1351-1370, http://www.irgrid.ac.cn/handle/1471x/1049576.[61] Lai, XiangJun, Li, Yan. Characteristics of convection and overshooting in RGB and AGB stars. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2011, 11(10): 1143-1157, http://lib.cqvip.com/Qikan/Article/Detail?id=39797287.[62] Su, Jie, Li, Yan. On the DB gap of white dwarf evolution: effects of hydrogen mass fraction and convective overshooting. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2010, 10(3): 266-278, http://lib.cqvip.com/Qikan/Article/Detail?id=33512762.[63] 李焱. 湍对流模型及其在恒星结构演化研究中的应用. 中国力学学会学术大会'2009论文摘要集. 2009, 170, http://www.irgrid.ac.cn/handle/1471x/1008050.[64] 张钱生, 李焱. Researching turbulent convection models and the density gradient reversing. IAU SYMPOSIUM PROCEEDINGS SERIES - ART OF MODELLING STARS IN THE 21ST CENTURY. 2008, 4(252): 133-134, http://www.irgrid.ac.cn/handle/1471x/1008072.[65] 刘忠, 金振宇, 林京, 李焱, 许骏. 30m环形干涉望远镜. 天文研究与技术[J]. 2006, 3(1): 64, http://lib.cqvip.com/Qikan/Article/Detail?id=21132411.[66] Liu Zhong, Jin Zhenyu, Li Yan, Lin Jing, Tan Huisong, Stepp LM. Introduction to the 30m Ring Interferometric Telescope. GROUND-BASED AND AIRBORNE TELESCOPES, PTS 1 AND 2. 2006, 6267: [67] 刘忠, 金振宇, 李焱, 林京, 谭徽松. Introduction to the 30m Ring Interferometric Telescope - art. no. 62672L. PROCEEDINGS OF THE SOCIETY OF PHOTO-OPTICAL INSTRUMENTATION ENGINEERS (SPIE) - GROUND-BASED AND AIRBORNE TELESCOPES, PTS 1 AND 2. 2006, 6267: L2672-L2672, http://www.irgrid.ac.cn/handle/1471x/1049141.[68] 郭建恒, 李焱. The correlation between the asymmetric mass loss and the Normal-SD phase of AG Car. ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES - STARS WITH THE BE PHENOMENON, PROCEEDINGS. 2006, 355: 207-209, http://www.irgrid.ac.cn/handle/1471x/1008069.[69] 杨家艳, 李焱. Testing Reynolds stress model in solar interior. PROCEEDINGS OF IAU SYMPOSIUM #239 - CONVECTION IN ASTROPHYSICS. 2006, 239: 373-375, http://www.irgrid.ac.cn/handle/1471x/1008070.[70] 刘忠, 金振宇, 林京, 李焱, 许骏. 30m环形干涉望远镜. 天文研究与技术国家天文台台刊[J]. 2006, 3(1): 64-72, http://lib.cqvip.com/Qikan/Article/Detail?id=21132411.[71] 郭建恒, 李焱, 单红光. A two-temperature model for LBVs. IAU SYMPOSIUM PROCEEDINGS SERIES - CORONAL AND STELLAR MASS EJECTIONS. 2005, 506-510, http://www.irgrid.ac.cn/handle/1471x/1008067.[72] 杨家艳, 李焱. NON-LOCAL CONVECTION THEORY ANDLTS APPLICATION TO SOLAR MODEL. 紫金山天文台台刊[J]. 2003, 22(2): 33-39, http://www.irgrid.ac.cn/handle/1471x/1049685.[73] 李焱. Convective overshooting to drive g-modes in gamma Dor stars. IAU SYMPOSIA - RECENT INSIGHTS INTO THE PHYSICS OF THE SUN AND HELIOSPHERE: HIGHLIGHTS FROM SOHO AND OTHER SPACE MISSIONS. 2001, 62-65, http://www.irgrid.ac.cn/handle/1471x/1008061.[74] 李焱, 杨家艳. Improved MLT and its applications to solar models. PROCEEDINGS OF IAU SYMPOSIUM - RECENT INSIGHTS INTO THE PHYSICS OF THE SUN AND HELIOSPHERE: HIGHLIGHTS FROM SOHO AND OTHER SPACE MISSIONS. 2001, 198-201, http://www.irgrid.ac.cn/handle/1471x/1008060.[75] 杨家艳, 李焱, 许华崟. Solar model with metal-enhanced convective envelope. PROCEEDINGS OF IAU SYMPOSIUM - RECENT INSIGHTS INTO THE PHYSICS OF THE SUN AND HELIOSPHERE: HIGHLIGHTS FROM SOHO AND OTHER SPACE MISSIONS. 2001, 46-49, http://www.irgrid.ac.cn/handle/1471x/1008059.[76] 龚志刚, 李焱. The Pulsations and Evolution of AGB Stars in the Large Magellanic Cloud. PROCCEEDINGSOFIAUSYMPOSIATHECARBONSTARPHENOMENON. 2000, 177: 199-204, http://www.irgrid.ac.cn/handle/1471x/1008044.[77] 杨家艳, 李焱, 许华. 外壳内金属丰度增加的非均匀太阳模型. 中国科学:A辑[J]. 2000, 30(12): 1141-1147, http://lib.cqvip.com/Qikan/Article/Detail?id=4799744.[78] 龚志刚, 袁永泉, 李焱, W.D ppen, 彭美仙. Research on the Solar Model and Oscillation in 1990s (II): Progress in Research on the Solar Oscillations. 天文学进展[J]. 1998, 16(4): 305-320, http://www.irgrid.ac.cn/handle/1471x/1050615.[79] 李焱. 恒星物质的不透明度. 天文学进展[J]. 1998, 16(2): 92, http://lib.cqvip.com/Qikan/Article/Detail?id=3065136.[80] 龚志刚, 李焱, Dappen W, 彭美仙, 袁永泉. 90年代太阳模型和太阳震荡研究进展i太阳模型研究进展. 天文学进展[J]. 1998, 16(4): 287, [81] 龚志刚, 袁永泉, W.D ppen, 李焱, 彭美仙. Research on the Solar Model and Oscillation in 1990s (I): Progress in Solar Models. 天文学进展[J]. 1998, 16(4): 287-304, http://www.irgrid.ac.cn/handle/1471x/1050614.[82] 龚志刚, 黄润乾, 李焱. 中等质量富金属AGB长周期变星的振动研究. 天体物理学报[J]. 1995, 15(1): 47, http://lib.cqvip.com/Qikan/Article/Detail?id=1902606.[83] 李焱, STIX, M. The δ Scuti instability strip: effects of opacity enhancement and wave reflections. ASTRONOMY & ASTROPHYSICS[J]. 1994, 286(3): 815-823, http://www.irgrid.ac.cn/handle/1471x/1049507.[84] 龚志刚, 李焱. 渐近巨星分支(AGB)长周期变星研究进展. 天文学进展[J]. 1994, 12(4): 320-332, http://www.irgrid.ac.cn/handle/1471x/1049633.[85] 李焱. The Red Edge of the Cepheid Instability Strip. PROCEEDINGS OF IAU COLLOQUIUM - NEW PERSPECTIVES ON STELLAR PULSATION AND PULSATING VARIABLE STARS. 1993, 139: 304-306, http://www.irgrid.ac.cn/handle/1471x/1008045.[86] 李焱. 恒星线性非绝热非径向脉动问题的退耦化处理方法. 天体物理学报[J]. 1989, 9(4): 345, http://lib.cqvip.com/Qikan/Article/Detail?id=149369.[87] 翟迪生, 陈海林, 李焱. 食双星船底ST(ST Car)和印第安RY(RY Ind)的光变曲线Roche模型分析. 天体物理学报[J]. 1988, 8(1): 20-25, http://www.irgrid.ac.cn/handle/1471x/1050172.