基本信息
李焱 男 汉族 博导 云南天文台
电子邮件:ly@ynao.ac.cn
联系电话:0871-3920768
手机号码:
通信地址:云南省昆明市东郊凤凰山中科院云南天文台
邮政编码:650011

研究领域

李焱,男,1963年6月出生于云南省昆明市;1983年毕业于北京大学地球物理系天体物理专业, 1989年获得中国科学院云南天文台天体物理专业硕士学位, 1992年获得中国科学院云南天文台天体物理专业博士学位;1993-1994年在德国Kiepenheuer太阳物理研究所访问,1996年开始任中国科学院云南天文台研究员,博士生导师,1998年入选人事部“百千万人才工程”第一、二层次,2001-2008年担任中国科学院国家天文台副台长和云南天文台台长,2006-2010年担任中国天文学会副理事长;主持和参加过多项国家973计划、国家自然科学基金和中国科学院项目,1996年获得国家杰出青年科学基金资助,1999-2002年主持国家自然科学基金重点项目,2001-2006年主持中国科学院创新工程重大项目;发表论文和专著40余篇,被SCI论文独立引用30余篇次;主要研究方向包括恒星结构演化、日震学与星震学等,目前研究兴趣主要集中在恒星内部的对流运动的描述,以及对流运动对恒星结构和演化的影响方面。

招生信息

   
招生专业
070401-天体物理
招生方向
恒星物理    恒星结构演化    恒星对流   
恒星物理    日震学              星震学

教育背景

   
学历
中科院云南天文台 -- 研究生
学位
中科院云南天文台 -- 博士

工作经历

   
工作简历
1996-01~现在, 中国科学院云南天文台, 研究员
1993-08~1995-12,中国科学院云南天文台, 副研究员
1989-08~1993-07,中国科学院云南天文台, 助理研究员
1983-08~1989-07,中国科学院云南天文台, 研究实习员

教授课程

恒星结构演化

恒星振动理论

出版信息

   
发表论文
[1] 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.
[2] 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.
[3] 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, [4] 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): [5] 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): [6] 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, https://www.webofscience.com/wos/woscc/full-record/WOS:000535885900040.
[7] 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.
[8] 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, [9] 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, [10] 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): https://www.webofscience.com/wos/woscc/full-record/WOS:000540537800001.
[11] 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, [12] 李焱. 一颗主序前盾牌座δ型变星IP Per的星震学. Astrophysical Journal. 2019, [13] 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.
[14] 李焱. 利用k-ω模型研究低质量恒星的对流超射. Astrophysical Journal. 2019, [15] 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, [16] 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.
[17] 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, [18] Chen, Xinghao, Li, Yan, Zhang, Xiaobin. Exploring the Convective Core of the Hybrid delta Scuti-gamma Doradus Star CoRoT 100866999 with Asteroseismology. ASTROPHYSICAL JOURNAL[J]. 2019, 887(2): http://dx.doi.org/10.3847/1538-4357/ab585b.
[19] 李焱. 慢脉动B型星HD 50230的高精度星震学. Astrophysical Journal. 2019, [20] 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.
[21] 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.
[22] 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.
[23] 李焱. 用星震学探索δ Scuti-γ Doradus型恒星CoRoT 100866999的对流核. Astrophysical Journal. 2019, [24] 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): 079803-1, http://lib.cqvip.com/Qikan/Article/Detail?id=675611515.
[25] 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): https://www.webofscience.com/wos/woscc/full-record/WOS:000440973300012.
[26] 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.
[27] 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.
[28] 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.
[29] Nikolay N. Samus, Yan Li. Preface: Stars and interstellar medium. 天文和天体物理学研究:英文版. 2018, 18(8): 1-3, http://lib.cqvip.com/Qikan/Article/Detail?id=676043901.
[30] 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): 49-1, http://lib.cqvip.com/Qikan/Article/Detail?id=7000843705.
[31] Samus, Nikolay N, Li, Yan. Preface: Stars and interstellar medium. RESEARCH IN ASTRONOMY AND ASTROPHYSICSnull. 2018, 18(8): http://lib.cqvip.com/Qikan/Article/Detail?id=676043901.
[32] 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.
[33] 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.
[34] Chen XueFei, Li Yan, Han ZhanWen. The formation of double compact objects as gravitational wave sources. SCIENTIA SINICA-PHYSICA MECHANICA & ASTRONOMICAnull. 2018, 48(7): [35] 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.
[36] 李焱. 采用k-omega模型处理sdB恒星中的对流超射. ApJ. 2018, [37] 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.
[38] 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 FUTUREnull. 2017, 160: [39] Li, Yan. Applications of the k-omega Model in Stellar Evolutionary Models. ASTROPHYSICAL JOURNAL[J]. 2017, 841(1): http://ir.ynao.ac.cn/handle/114a53/10070.
[40] 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.
[41] 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.
[42] 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://ir.ynao.ac.cn/handle/114a53/9923.
[43] 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. EPJ Web of Conferences - SEISMOLOGY OF THE SUN AND THE DISTANT STARS 2016-USING TODAY'S SUCCESSES TO PREPARE THE FUTUREnull. 2017, 160: 1-4, [44] 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 WORKSHOPnull. 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.
[45] 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.
[46] 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.
[47] 郭志亮, 李焱. 恒星对流k-w模型的性质研究. 天文学报[J]. 2014, 55(1): 66-77, [48] 郭志亮, 李焱. 恒星对流k—ω模型的性质研究. 天文学报. 2014, 55(1): 66-77, http://lib.cqvip.com/Qikan/Article/Detail?id=48436813.
[49] 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.
[50] 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.
[51] 李焱. 恒星对流的k-omega模型. 2013中国天文学会学术年会文集null. 2013, 45-, http://www.irgrid.ac.cn/handle/1471x/1008054.
[52] 张瑞玉, 李焱. 存在非同步转动的双星演化模型. 天文学报. 2012, 53(4): 274-290, http://lib.cqvip.com/Qikan/Article/Detail?id=42819958.
[53] 李焱. 恒星湍热对流的k-omega模型. ApJ. 2012, [54] 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.
[55] 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.
[56] 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.
[57] 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.
[58] 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null. 2009, 170-, http://www.irgrid.ac.cn/handle/1471x/1008050.
[59] 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 CENTURYnull. 2008, 4(252): 133-134, http://www.irgrid.ac.cn/handle/1471x/1008072.
[60] 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. 2006, 3(1): 64-72, http://lib.cqvip.com/Qikan/Article/Detail?id=21132411.
[61] 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 2null. 2006, 6267: [62] 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, Proceedingsnull. 2006, 355: 207-209, http://www.irgrid.ac.cn/handle/1471x/1008069.
[63] 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 2null. 2006, 6267: L2672-L2672, http://www.irgrid.ac.cn/handle/1471x/1049141.
[64] 杨家艳, 李焱. Testing Reynolds stress model in solar interior. Proceedings of IAU Symposium #239 - Convection in Astrophysicsnull. 2006, 239: 373-375, http://www.irgrid.ac.cn/handle/1471x/1008070.
[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:国家天文台台刊. 2006, 3(1): 64-72, http://lib.cqvip.com/Qikan/Article/Detail?id=21132411.
[66] 郭建恒, 李焱, 单红光. A two-temperature model for LBVs. IAU Symposium Proceedings Series - CORONAL AND STELLAR MASS EJECTIONSnull. 2005, 506-510, http://www.irgrid.ac.cn/handle/1471x/1008067.
[67] 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.
[68] 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 MISSIONSnull. 2001, 62-65, http://www.irgrid.ac.cn/handle/1471x/1008061.
[69] 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 MISSIONSnull. 2001, 198-201, http://www.irgrid.ac.cn/handle/1471x/1008060.
[70] 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 MISSIONSnull. 2001, 46-49, http://www.irgrid.ac.cn/handle/1471x/1008059.
[71] 龚志刚, 李焱. The Pulsations and Evolution of AGB Stars in the Large Magellanic Cloud. Procceedings of IAU Symposia - The Carbon Star Phenomenonnull. 2000, 177: 199-204, http://www.irgrid.ac.cn/handle/1471x/1008044.
[72] 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. 2000, 30(12): 1141-1147, http://lib.cqvip.com/Qikan/Article/Detail?id=4799744.
[73] 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.
[74] 李焱. 恒星物质的不透明度. 天文学进展. 1998, 16(2): 92-102, http://lib.cqvip.com/Qikan/Article/Detail?id=3065136.
[75] 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.
[76] 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-, [77] 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. 1995, 15(1): 47-56, http://lib.cqvip.com/Qikan/Article/Detail?id=1902606.
[78] 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.
[79] 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.
[80] 李焱. The Red Edge of the Cepheid Instability Strip. Proceedings of IAU Colloquium - NEW PERSPECTIVES ON STELLAR PULSATION AND PULSATING VARIABLE STARSnull. 1993, 139: 304-306, http://www.irgrid.ac.cn/handle/1471x/1008045.
[81] 李焱. 星风物质损失对造父变星脉动性质的影响. 1989, 63-, http://ir.ynao.ac.cn/handle/114a53/5306.
[82] 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): 345-352, http://www.irgrid.ac.cn/handle/1471x/1049629.
[83] 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.
发表著作
(1) 恒星结构演化引论, Introduction of stellar structure and evolution, 北京大学出版社, 2014-04, 第 1 作者

科研活动

   
科研项目
( 1 ) 恒星对流超射区湍流性质与对流混合研究, 主持, 国家级, 2010-01--2012-12
( 2 ) 恒星对流与磁场研究, 主持, 国家级, 2014-01--2018-12

指导学生

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杨家艳  博士研究生  070401-天体物理  

郭建恒  博士研究生  070401-天体物理  

余聪  博士研究生  070401-天体物理  

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丁彩云  博士研究生  070401-天体物理  

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苏杰  博士研究生  070401-天体物理  

房祥松  博士研究生  070401-天体物理  

张钱生  博士研究生  070401-天体物理  

郭志亮  硕士研究生  070401-天体物理  

吴涛  博士研究生  070401-天体物理  

陈彦辉  博士研究生  070401-天体物理  

郭军军  博士研究生  070401-天体物理  

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李华居  博士研究生  070401-天体物理  

张昕旖  博士研究生  070401-天体物理  

郭飞  博士研究生  070401-天体物理  

邢磊  博士研究生  070401-天体物理  

李志  博士研究生  070401-天体物理  

王悦同  博士研究生  070401-天体物理  

李雪峰  硕士研究生  070401-天体物理