王博
?中国科学院云南天文台，研究员、博导
通信地址： 云南省昆明市东郊凤凰山云南天文台
邮政编码： 650216
电子邮件：wangbo@ynao.ac.cn
电 话：+86- (office)
传 真：+86-
简历
工作简历：
2016/06 - 至今 中国科学院云南天文台 博导
2015/05 - 至今 中国科学院云南天文台 研究员
2012/02 - 2015/04 中国科学院云南天文台 副研究员
2010/07 - 2012/01 中国科学院云南天文台 助理研究员
学习简历：
2005/09 - 2010/07 中国科学院云南天文台 博士
2001/09 - 2005/07 云南大学物理系 学士
研究领域
研究领域主要涉及恒星物理、双星演化、大样本恒星演化、特殊恒星及相关天体，特别是Ia型超新星前身星的研究。Ia型超新星是宇宙学距离指示器，通过Ia型超新星测距，波尔马特等人发现了宇宙在加速膨胀，从而推论出暗能量的存在。暗能量的发现不仅是天文学，更是物理学的巨大突破（波尔马特等人由此获得了2011年度诺贝尔物理学奖）。然而，人们并不清楚Ia型超新星的前身星是什么，这将直接影响Ia型超新星的测距精度并阻碍精确宇宙学的发展。在Ia型超新星前身星及其相关天体方面开展了一系列，提出了Ia型超新星的氦双星前身星模型，成功地揭示了年轻Ia型超新星如何形成的难题，受到英、美、德、俄、葡等30多个国家70余家国外媒体(如BBC, Science Daily)的报道，并被《Nature》杂志主办的《Nature China》作为研究亮点进行报道。氦双星模型现已被广泛应用于Ia型超新星的爆炸模型研究。近年来，进一步发展了氦双星模型，发现白矮星吸积氦亚巨星是形成大质量双白矮星系统最有效的途径，进一步限制了Ia型超新星爆炸后残留伴星的特征,为国际上众多搜寻 Ia 型超新星残留伴星的大型巡天项目提供了理论依据。发表的论文被Nature等30余篇权威期刊评述及引用，研究成果写入Springer出版社《超新星手册》等5部专著，并被选入《十二五国家基金资助项目优秀成果选编》。
获奖及荣誉
(1)国家优秀青年科学基金获得者（2013年）
(2)国家自然科学奖二等奖（2013年），排名第四
(3)2019年获首批云南省科学基金
(4)2019年获中科院优秀导师奖
(5)2018年获首批云南省“”拔尖人才
(6)2018年获云南省中青年学术与技术带头人荣誉称号
(7)2017年获中科院大学必和必拓导师科研奖
(8)2016年获中科院前沿科学重点研究计划（拔尖青年科学家类）支持
(9)2013年获中科院公派出国留学计划“高级研究”项目
(10) 2011年获中科院卢嘉锡青年人才奖
(11) 2011年获中科院优秀博士论文奖
(12) 2011年入选首批中科院青年创新促进会成员（2015年首批优秀会员）
(13) 2011年获云南省优秀科技论文特等奖，排名第一
(14) 2010年获中科院院长特别奖
(15) 2009年获云南省优秀科技论文一等奖，排名第一
(16) 2009年度中国十大天文科技进展（主要完成人）
科研项目
(1)主持中科院前沿科学重点研究计划（拔尖青年科学家类）1项（2016-2021）
(2)国家基金“恒星物理”创新群体，核心成员（共5人，2016-2021）
(3)主持云南省“”拔尖人才专项（2019-2023）
(4)主持首批云南省科学基金1项（2019-2022）
(5)主持国家基金面上项目1项（2019-2022）
(6)主持国家基金面上项目1项（2017-2020）
(7)主持中科院青促会优秀会员人才专项（2016-2018）
(8)主持国家基金优秀青年科学基金1项（2014-2016）
(9)主持国家基金青年科学基金1项（2012-2014）
(10)主持中科院青促会人才专项（2011-2014）
(11)主持中科院“西部之光”博士资助项目1项（2011-2013）
(12)参与国家基金重大项目1项，骨干（2014-2018）
(13)参与科技部973项目: 基于LAMOST大科学装置的银河系研究及多波段天体证认，骨干（2014-2018）
(14)参与科技部973项目: 黑洞以及其它致密天体物理的研究，骨干（2011-2013）
论文列表
Pulished papers (please click theADS libraryfor the latest list)
(1)WangB., Han Z., Progenitors of type Ia supernovae, 2012, New Astronomy Reviews, 56, pp122-141 (特邀评述)
(2)Wang B., Mass-accreting white dwarfs and type Ia supernovae，2018, Res. Astron. Astrophys., 18, 49 (特邀评述)
(3)Wang B., The single-degenerate model for the progenitors of accretion-induced collapse events，2018, MNRAS, 481, pp439–446
(4)Wang B., Podsiadlowski P., Han Z., He-accreting carbon-oxygen white dwarfs and type Ia supernovae, 2017, MNRAS, 472, pp1593–1599
(5)Wang B., Zhou W., Zuo Z., Li Y., Luo X., Zhang J., Liu D., Wu C., The core-degenerate scenario for the progenitors of type Ia supernovae, 2017, MNRAS, 464, pp3965-3971
(6)Wang B., Li Y., Ma X., Liu D., Cui X., Han Z., Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs, 2015, A&A, 584, A37
(7)Wang B., Ma X., Liu D.-D., Liu Z., Wu C.-Y., Zhang J., Han Z., Super-Eddington wind scenario for progenitors of type Ia supernovae: binary population synthesis calculations, 2015, A&A, 576, A86
(8)Wang B., Meng X., Liu D., Liu Z., Han Z., The hybrid CONe WD + He star scenario for the progenitors of type Ia supernovae, 2014, ApJ Letters, 794, L28
(9)WangB., JusthamS., Liu Z., Zhang J., Liu D., Han Z., On the evolution of rotating accreting white dwarfs and type Ia supernovae, 2014, MNRAS, 445, pp2340-2352
(10)WangB., JusthamS., Han Z., Producing type Iax supernovae from a specific class of helium-ignited WD explosions, 2013, A&A, 559, A94
(11)Wang B., Li X.-D., Han Z., The progenitors of type Ia supernovae with long delay times, 2010, MNRAS, 401, pp2729-2738
(12)Wang B., Han Z., Companion stars of type Ia supernovae and single low-mass white dwarfs, 2010, MNRAS, 404, L84-L88
(13)Wang B., Han Z., The helium star donor channel for the progenitors of type Ia supernovae with different metallicities, 2010, A&A, 515, A88
(14)Wang B., Meng X., Chen X., Han Z., The helium star donor channel for the progenitors of type Ia supernovae, 2009, MNRAS, 395, pp847-854
(15)Wang B., Chen X., Meng X., Han Z., Evolving to type Ia supernovae with short delay times, 2009, ApJ, 701, pp1540-1546
(16)Wang B., Han Z., Companion stars of type Ia supernovae and hypervelocity stars, 2009, A&A, 508, L27-L30
(17)WangB., Han Z., WD+RG systems as the progenitors of type Ia supernovae, 2010, Res. Astron. Astrophys., 10, pp235-243
(18)Wang B., Liu Z., Han Y., Lei Z., Luo Y., Han Z., Birthrates and delay times of type Ia supernovae, 2010, Science China Physics, Mechanics & Astronomy, 53, pp586-590
(19)Wang B., Han Z., WD + He star systems as the progenitors of type Ia supernovae and their surviving companion stars, 2010, Ap&SS, 329, pp293-296
(20)Wang B., Han Z., A likely candidate of type Ia supernova progenitors: the X-ray pulsating companion of the hot subdwarf HD 49798, 2010, Res. Astron. Astrophys., 10, pp681-688
(21)WangB., MengX., WangX.-F., Han Z., Distribution of Ni yields of type Ia supernovae and its implication for progenitors, 2008, Chin. J. Astro. Astrophys., 8, pp71-80
(22)Tang W., Liu D., Wang B.*, Evolving neutron star+helium star systems to intermediate-mass binary pulsars, 2019, MNRAS, 490, pp752-757 (*通讯作者)
(23)Wu C., Wang B.*, Off-centre carbon burning in He-accreting carbon-oxygen white dwarfs, 2019, MNRAS, 486, pp2977- 2981 (*通讯作者)
(24)Liu D., Wang B.*, Ge H., Chen X., Han Z., The progenitors of type Ia supernovae in the semidetached binaries with red giant donors, 2019, A&A, 622, A35 (*通讯作者)
(25)Wu C., Wang B.*, Liu D., The outcomes of carbon-oxygen white dwarfs accreting CO-rich material, 2019, MNRAS, 483, pp263-275 (*通讯作者)
(26)Wu D., Liu D., Wang B.*, Past and future of the central double-degenerate core of Henize 2-428, 2019, Res. Astron. Astrophys., 19, 57 (*通讯作者)
(27)Liu D., Wang B.*, Chen W., Zuo Z., Han Z., Evolving ONe WD+He star systems to intermediate-mass binary pulsars, 2018, MNRAS, 477, pp384–391 (*通讯作者)
(28)Wu C., Wang B.*, Accreting CO material onto ONe white dwarfs towards accretion-induced collapse, 2018, Res. Astron. Astrophys., 18, id.36 (*通讯作者)
(29)Liu D., Wang B.*, Han Z., The double-degenerate model for the progenitors of type Ia supernovae, 2018, MNRAS, 473, pp5352–5361 (*通讯作者)
(30)Liu D., Wang B.*, Wu C., Han Z., Merging of a CO WD and a He-rich WD to produce a type Ia supernovae, 2017, A&A, 606, A136 (*通讯作者)
(31)Wu C., Wang B.*, Liu D., Han Z., Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae, 2017, A&A, 604, A31(*通讯作者)
(32)Liu D., Wang B.*, Podsiadlowski P., Han Z., The violent white dwarf merger scenario for the progenitors of type Ia supernovae, 2016, MNRAS, 461, pp3653-3662 (*通讯作者)
(33)Wu C., Liu D., Zhou W., Wang B.*, Accreting He-rich material onto carbon-oxygen white dwarfs until explosive carbon ignition, 2016, Res. Astron. Astrophys., 16, id.160 (*通讯作者)
(34)Liu D., Zhou W., Wu C., Wang B.*, Is the X-ray pulsating companion of HD 49798 a possible type Ia supernova progenitor? 2015, Res. Astron. Astrophys., 15, pp1813-1822(*通讯作者)
(35)Zhou W., Wang B.*, Meng X., Liu D., Zhao G., Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors, 2015, Res. Astron. Astrophys., 10, pp1701-1712 (*通讯作者)
(36)Zhou W., Wang B.*, Zhao G., Double-detonation model of type Ia supernovae with a variable helium layer ignition mass, 2014, Res. Astron. Astrophys., 14, pp1146-1156 (*通讯作者)
(37)Cui X., Wang B., Wu C., Meng X., Han Z., The C/O ratio of He-accreting carbon-oxygen white dwarfs and type Ia supernovae, 2020, Res. Astron. Astrophys., 20, 3
(38)Moriya T. J., Liu D., Wang B., Liu Z., Circumstellar properties of Type Ia supernovae from the helium star donor channel, 2019, MNRAS, 488, pp3949-3956
(39)Yu Y., Chen A., Wang B., Optical and radio transients after collapse of super-Chandrasekhar white dwarf merger remnants, 2019, ApJ Letters, 870, L23
(40)Li Y.-P., Yuan F., Mo H.-J., Yoon D., Gan Z., Ho L. C., Wang B., Ostriker J. P., Ciotti L., Stellar and AGN Feedback in Isolated Early-type Galaxies: The Role in Regulating Star Formation and ISM Properties, 2018, ApJ, 866, 70
(41)Li Y.-B., Luo A., Du C., Zuo F., Wang M., Zhao G., Jiang B., Zhang H., Liu C., Qin L., Wang R., Du B., Guo Y., Wang B., Han Z., Xiang M., Huang Y., Chen B., Chen J., Kong X., Hou W., Song Y., Wang Y., Wu K., Zhang J., Zhang Y., Wang Y., Cao Z., Hou Y., Zhao Y., Carbon stars identified from LAMOST DR4 using Machine Learning, 2018, ApJS, 234, id.31
(42)Huang Y., Liu X., Zhang H., Chen B., Xiang M., Wang C., Yuan H., Tian Z., Li Y., Wang B., Discovery of Two New Hypervelocity Stars from the LAMOST Spectroscopic Surveys, 2017, ApJ Letters, 847, L9
(43)Zhang J., Wang X., Sasdelli M., Zhang T., Liu Z., Mazzali P. A., Meng X., Maeda K., Chen J., Huang F., Zhao X., Zhang K., Zhai Q., Pian E., Wang B. et al., A Luminous Peculiar Type Ia Supernova SN 2011hr: More Like SN 1991T or SN 2007if? 2016, ApJ, 817, 114
(44)Geier S., Fürst F., Ziegerer E., Kupfer T., Heber U., Irrgang A., Wang B., Liu Z., Han Z., Sesar B., Levitan D., Kotak R., Magnier E., Smith K., Burgett W. S., Chambers K., Flewelling H., Kaiser N., Wainscoat R., Waters C., The fastest unbound star in our Galaxy ejected by a thermonuclear supernova, 2015, Science, 347, pp1126?–?1128
(45)Liu Z., Stancliffe R. J., Abate C., Wang B., Pre-explosion companion stars in Type Iax supernovae, 2015, ApJ, 808, 138
(46)Li Y., Luo A., Zhao G., Lu Y., Wei P., Du B., Li X., Zhao Y., Han Z., Wang B., Wu Y., Zhang, Y., Hou Y., Wang Y., Yang M., 19 low mass hyper-velocity star candidates from the first data release of LAMOST survey, 2015, Res. Astron. Astrophys., 15, pp1364-1377
(47)LiuZ., Moriya Takashi J., Stancliffe Richard J., WangB., Constraints on single-degenerate Chandrasekhar mass progenitors of Type Iax supernovae, 2015, A&A, 574, A12
(48)Zhang J., Wang X., Bai J., Zhang T., Wang B., Liu Z., Zhao X., Chen J., Optical and Ultraviolet Observations of the Narrow-Lined Type Ia SN 2012fr in NGC 1365, 2014, AJ, 148, 1
(49)Liu Z., Pakmor R., Roepke F. K., Edelmann P., Hillebrandt W., Kerzendorf W. E., Wang B., Han Z., Rotation of surviving companion stars after type Ia supernova explosions in the WD+MS scenario, 2013, A&A, 554, A109
(50)Liu Z., Pakmor R., SeitenzahlI.R., Hillebrandt W., KromerM., Roepke F. K., Edelmann P., TaubenbergerS., MaedaK., Wang B., Han Z., The Impact of Type Ia Supernova Explosions on Helium Companions in the Chandrasekhar-mass Explosion Scenario, 2013, ApJ, 774, 37
(51)Liu Z., Kromer M., Fink M., Pakmor R., Roepke F. K., Chen X., Wang B., Han Z., Predicting the Amount of Hydrogen Stripped by the SN Explosion for SN 2002cx-like SNeIa, 2013, ApJ, 778, 121
(52)GeierS., MarshT.R., WangB., Dunlap B., Barlow B. N., Schaffenroth V., Chen X., Irrgang A., Maxted P. F. L., Ziegerer E., Kupfer T., Miszalski B., Heber U., Han Z., Shporer A., Telting J. H., G?nsicke B. T., ?stensen R. H., O'Toole S. J., Napiwotzki R., A progenitor binary and an ejected mass donor remnant of faint type Ia supernovae, 2013, A&A, 554, A54
(53)Zhang J., Wang B., Zhang B., Han Z., Reanalysis of the isotopic mixture of neutron-capture elements in the metal-poor Star HD 175305, 2012, Chinese Physics Letters, 29, 019701
(54)Luo Y., Wang B., Chen H., Zhang X., Han Z., Photometric analysis of a blue straggler eclipsing binary in the old open cluster NGC 2141, 2012, Science China Physics, Mechanics & Astronomy, 55, pp1500-1504
(55)Han Y., Dai B., Wang B., Zhang F., Han Z., Evolution of luminosity function and obscuration of AGN: connecting X-ray and Infrared, 2012, MNRAS, 423, pp464-477
(56)Deng L., Newberg H. J., Liu C., CarlinJ.L., BeersT.C., ChenL., ChenY., ChristliebN., GrillmairC.J., Guhathakurta P., HanZ., HouJ., LeeH.-T., Lépine S., LiJ., Liu X., Pan K., SellwoodJ.A., WangB., WangH., Yang F., YannyB., ZhangH., Zhang Y., ZhengZ., ZhuZ., LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) — The survey’s science plan, 2012, Res. Astron. Astrophys, 123, pp735-754
(57)Liu Z., Pakmor R., Roepke F. K., Edelmann P., Wang B., Kromer M., Hillebrandt W., Han Z., Three-dimensional simulations of interaction between type Ia supernova ejecta and their main sequence companions, 2012, A&A, 548, A2
(58)LiuW., ChenW., WangB., HanZ., Helium star evolutionary channel to super-Chandrasekhar mass type Ia supernovae, 2010, A&A, 523, A3
指导学生已指导学生
刘栋栋博士研究生070401-天体物理
吴程远博士研究生070401-天体物理
吴东昊硕士研究生070401-天体物理
现指导学生
唐文师硕士研究生070401-天体物理
魏丹丹博士研究生070401-天体物理
郭云浪硕士研究生070401-天体物理
招生信息
天体物理：恒星物理, 双星演化, 大样本恒星演化, 特殊恒星及相关天体，超新星前身星
招生专业070401-天体物理
招生方向恒星物理
