杨伍明 - 北京师范大学

个人简介

学历、工作经历 1997.9 － 2002.7，云南大学，物理系，数理基地专业，学士 2002.9 － 2007.7，中科院云南天文台，天体物理专业，博士 2007.7 － 2012.8，河南理工大学理化学院，讲师—副教授 2012.9 －今，北京师范大学大天文系，讲师—副教授项目恒星演化对星团主序拐点扩展的影响研究，国家基金面上项目，2018.1, 主持，在研国家基金天文联合基金重点项目：U1631236，参与大样本红团簇巨星的类太阳星振研究，国家基金面上项目，2013.1-2016.12, 主持，结题主讲课程热力学统计物理，本科星震学，研究生

研究领域

1、恒星结构和演化及星团研究 a. 从2004－2018的十余年间，恒星物理学者无法构造出和日震反演和中微子预测相一致的低金属丰度太阳模型。我们提出利用转动演化太阳模型－－动力学太阳模型来解决，给出低金属丰度的转动太阳模型很好地再现了日震学反演结果和中微子探测结果。 b.星团颜色星等图的研究。我们的转动恒星演化模型预测的星团颜色星等图主序拐点扩展随年龄变化被观测证实(Yang et al.2013, ApJ,776,112)。 2、星振学人类有能力建造越来越大的望远镜，观测到越来越远的天体。但再大的望远镜也无法看穿太阳和恒星表面的阻碍。获得和理解隐藏在恒星表面下的结构和物理过程一直是天文学追求的重要目标。我们建立起了星振学观测诊断恒星对流核的理论。第一个给出观测确定恒星对流核大小的星振学方法。之前天文学对恒星内核的认识几乎都来源于理论模型而非实验观测。我们的研究的意义在于第一次使人们对恒星内核的认识和理解直接来自观测实验而非理论模型计算。

近期论文

查看导师最新文章（温馨提示：请注意重名现象，建议点开原文通过作者单位确认）

杨伍明，Rotating Solar Models with Low Metal Abundances as Good as Those with High Metal Abundances，2019, ApJ, in press 杨伍明，The Effects of Binary Stars on the Color-magnitude Diagrams of Young-age Massive Star Clusters，2018, ApJ，860, 132 杨伍明,Tian Z., The effects of the overshooting of the convective core on main-sequence turnoffs of young- and intermediate-age star clusters, ApJ, 2017, 836，102 杨伍明, Estimate the radius of the convective core of main-sequence stars from observed oscillation frequencies, ApJ, 2016,829,68 杨伍明, Solar models with new low-metal abundances, ApJ, 2016,821,108 杨伍明, Tian Z., Bi S., Ge Z., Wu Y., and Zhang J., Asteroseismic Analysis of Kepler Target 2837475, MNRAS, 2015, 453, 2094 Liu Z., 杨伍明(通讯作者), Bi S. et al., Asteroseismic Analysis of the CoRoT Target HD49933, ApJ, 2014, 780, 152 杨伍明, Bi S., Meng X.等，The effects of rotation on the main-sequence turnoff of intermediate-age massive star clusters，ApJ，2013, 776, 112 杨伍明, Bi S., Meng X.等，Evolution of Rotational Velocities of A-type Stars，ApJL, 2013, 765, L36 杨伍明, Bi S., Meng X.，Grids of rotating stellar models with masses between 1.0 and 3.0 Msun，RAA，2013, 13, 579 杨伍明, Meng X.，Bi S.等，Characteristics of solar-like oscillations of secondary red-clump stars，MNRAS，2012, 422, 1552 杨伍明, Li Z., Meng X., Bi S.，Characteristics of solar-like oscillations of clusters simulated by stellar population synthesis，MNRAS，2011，414，1769 杨伍明, Meng X., Bi S.等，The contributions of interactive binary stars to double main-sequence turnoffs and dual red clump of intermediate-age star clusters, ApJL，2011，731，L37 杨伍明, Meng X., Li Z.等，The effects of stellar population synthesis on the distributions of the asteroseismic observables νmax and Δν of red-clump stars，MNRAS，2010，409，873 杨伍明, Meng X., Models of μ Her with asteroseismic constraints, NewA., 2010, 15, 367 杨伍明, Meng X., Frequency Separation Variations of the Solar Low-Degree p-Modes, PASJ, 2009, 61, 1399 杨伍明, Bi S.，Rotation Profiles of Solar-like Stars with Magnetic Fields， Chjaa， 2008， 8, 677 杨伍明, Li M., Asteroseismic constraints on the OPAL opacity interpolation，IAUS, 2008, 252, 123 杨伍明, Bi S., Solar Models with Revised Abundances and Opacities, ApJL, 2007, 685, L67 杨伍明, Bi S.，The frequency separations of stellar p-modes，A&A，2007, 472, 571 杨伍明, Bi S., Angular Momentum Transport and Element Mixing in the Stellar Interior. I. Application to the Rotating Sun, A&A, 2006, 449, 1161 Meng X.，杨伍明, The birth rate of supernovae from double-degenerate and core-degenerate systems，A&A，2012, 543, A137 Meng X., 杨伍明, The correlation between C/O ratio, metallicity, and the initial WD mass for SNe Ia, 2011, A&A, 531, A94 Meng X., 杨伍明, Binary population synthesis study of the supersoft X-ray phase of single degenerate type Ia supernova progenitors, 2011，RAA，11，965 Meng X., 杨伍明, The companion properties of SNe Ia from the single degenerate model，中国科学G，2011，54，2296 Meng X., 杨伍明, A Comprehensive Progenitor Model for SNe Ia, ApJ, 2010, 710, 1310-1323 Meng X., 杨伍明, Companion stars of Type Ia supernovae with different metallicities, MNRAS, 2010, 401, 1118-1130 Meng X., 杨伍明, The envelope mass of red giant donors in Type Ia supernova progenitors, A&A, 2010, 516A, 47 Meng X., 杨伍明, WD+MS systems as the progenitor of SNe Ia, Ap&SS, 2010, 329, 287 Meng X., 杨伍明, Geng X., Is SN 2006X from a WD + MS system with optically thick wind? NewA, 2010, 15, 343-345 Meng X., 杨伍明, Li Z.，The cooling time of white dwarfs produced from type Ia supernovae, RAA，2010，10，927 Meng X., 杨伍明, Li Z., The initial and final state of SNe Ia from the single degenerate model，中国科学G，2010， 53，1732 Meng X., 杨伍明, Geng X., WD+MS Systems as Progenitors of Type Ia Supernovae with Different Metallicities, PASJ, 2009, 61, 1251－1260 Bi S., 杨伍明, Solar Model Including Magnetic Fields and Rotation，AIPC, 2007, 948, 309-313 Meng X.,Li Z.，杨伍明, The Effect of Metallicity on the Delay-Time Distribution of Type Ia Supernova, 2011，PASJ，63，L31 Meng X., Cheng W., 杨伍明, Li Z., The birth rate of subluminous and overluminous type Ia supernovae，2011，A&A, 525A, 129 Li, T. D.，Bi, S. L.，杨伍明，Liu, K.，Tian, Z. J.，Ge, Z. S.，Effects of Magnetic Fields on Lithium Evolution in F and G Stars，ApJ，2014, 781, 62 Tian, Z. J., Bi, S. L., 杨伍明等, Asteroseismic analysis of solar-like star KIC 6225718: constraints on stellar parameters and core overshooting, MNRAS, 2014, 445, 2999 Liu, Zhi-E.; Bi, Shao-Lan; 杨伍明等，Exploring the sources of p-mode frequency shifts in the CoRoT target HD 49933，RAA，2014, 14, 683 Bi, S. L.; Li, T. D.; Li, L. H.; 杨伍明，Solar Models with Revised Abundance，ApJL，2011，731，L42 Meng Xiang-Cun, Chen Xue-Fei, Han Zhan-Wen, 杨伍明，Color excesses of type Ia supernovae from the single-degenerate channel model，RAA，2009，9，1259-1269 Tian, Zhijia; Bi, Shaolan; Bedding, Timothy R.; 杨伍明, Asteroseismic analysis of solar-mass subgiants KIC 6442183 and KIC 11137075 observed by Kepler, 2015, A&A, 580, 44 Ge, Z. S.; Bi, S. L.; Li, T. D.; Liu, K.; Tian, Z. J.; 杨伍明; Liu, Z. E.; Yu, J.，Asteroseismic analysis of two alpha-enhanced stars KIC 7976303 and KIC 8694723，2015, MNRAS, 2015, 447, 680