黄永锋
近期热点
资料介绍
个人简历
1972年1月生,湖北新洲人。1994年6月南京大学天文系本科毕业,1999年6月于南京大学天文系获得博士学位。1999年8月起留校工作,现为教授、博士生导师,2006年度国家杰出青年科学基金获得者,是江苏省“333高层次人才培养工程”第二层次培养对象。曾获得全国优秀博士学位论文奖、教育部自然科学奖一等奖、国家自然科学二等奖、天文学会黄授书奖等。承担课程曾经在天文学系讲授《实测天体物理》、《近代天文讲座》、《现代天文科研入门》等课程。2016年起主要承担《热力学 统计物理》课程的教学工作。到2018年10月,已发表SCI论文107篇,研究论文已被国内外同行他引逾1300篇次。2006年获得国家杰出青年科学基金资助,还曾主持过全国优秀博士学位论文作者专项基金和自然科学基金青年项目、面上项目等,2009-2013曾担任973项目课题组长。截止2018年10月,已指导博士毕业5人,指导硕士毕业十余人。研究领域
"主要从事高能天体物理尤其是宇宙伽玛射线暴、中子星、脉冲星、快速射电暴等的研究"近期论文
[1] Huang Y.F., Lu T., 1997, Chinese Physics Letters, 14, 314 -- 316: “On the crust of a strange star”[2] Huang Y.F., Lu T., 1997, A&A, 325, 189 --- 194: “Strange stars: how dense can their crust be?”[3] Huang Y.F., Dai Z.G., Wei D.M., Lu T., 1998, MNRAS, 298, 459 -- 463: “Gamma-ray bursts: post-burst evolution of fireballs”[4] Huang Y.F., Dai Z.G., Lu T., 1998, A&A, 336, L69 -- L72: ”GRB afterglows: from ultra-relativistic to non-relativistic phase” [5] Huang Y.F., Dai Z.G., Lu T., 1998, Chinese Physics Letters, 15, 775 -- 777: “Fireball/blastwave model and soft gamma-ray repeaters” [6] Dai Z.G., Huang Y.F., Lu T., 1999, ApJ, 520, 634 -- 640: ”Gamma-ray burst afterglows from realistic fireballs”[7] Huang Y.F., Dai Z.G., Lu T., 1999, MNRAS, 309, 513 -- 516: “A generic dynamical model of gamma-ray burst remnants”[8] Huang Y.F., Dai Z.G., Lu T., 1999, Chinese Physics Letters, 16, 775 -- 777: “Overall evolution of realistic gamma-ray burst remnant and its afterglow”[9] Huang Y.F., Dai Z.G., Lu T., 2000, A&A, 355, L43 -- L46: “Rapid fading of optical afterglows as evidence for beaming in gamma-ray bursts” [10] Huang Y.F., Dai Z.G., Lu T., 2000, Chinese Physics Letters, 17, 778 -- 780: “Afterglows from jetted gamma-ray burst remnant: does the light curve break?”[11] Huang Y.F., Dai Z.G., Lu T., 2000, MNRAS, 316, 943 -- 949: “On the optical light curves of afterglows from jetted gamma-ray burst ejecta: effects of parameters” [12] Huang Y.F., Gou L.J., Dai Z.G., Lu T., ApJ, 2000, 543, 90 -- 96: “Overall evolution of jetted gamma-ray burst ejecta” [13] Wang X.Y., Dai Z.G., Lu T., Wei D.M., Huang Y.F., 2000, A&A, 357, 543 -- 547: “A possible model for the supernova/gamma-ray burst connection”[14] Gou L.J., Dai Z.G., Huang Y.F., Lu T., 2001, A&A, 368, 464 -- 470: “Gamma-ray burst afterglows from jetted shocks in wind environments” [15] Cheng K.S., Huang Y.F., Lu T., 2001, MNRAS, 325, 599 -- 606: “Gamma-ray bursts: afterglows from cylindrical jets”[16] Dai Z.G., Huang Y.F., Lu T., 2001, MNRAS, 324, L11 -- L15: “Light curves of jetted gamma-ray burst afterglows in circumstellar clouds”[17] Gou L.J., Dai Z.G., Huang Y.F., Lu T., 2001, Chinese Astron. Astr., 25, 29 -- 40: “The joint effect of jet and stellar wind on GRB afterglow” [18] Huang Y.F., Tan C.Y., Dai Z.G., Lu T., 2002, Chinese Astronomy and Astrophysics, 26, 414 -- 423: “Are gamma-ray bursts due to isotropic fireballs or cylindrical jets?” [19] Huang Y.F., Dai Z.G., Lu T., 2002, MNRAS, 332, 735 -- 740: “Failed gamma-ray bursts and orphan afterglows” [20] Ma Z.X., Dai Z.G., Huang Y.F., Lu T., 2002, Astrophysics and Space Science, 282, 537 -- 550: “The crust properties and cooling of strange stars”[21] Feng J.B., Huang Y.F., Dai Z.G., Lu T., 2002., Chin. J. Astron. Astrophys., 2, 525 -- 532: “Dynamical evolution of gamma-ray burst remnants with evolving radiative efficiency” [22] Fan Y.Z., Dai Z.G., Huang Y.F., Lu T., 2002, Chin. J. Astron. Astrophys., 2, 449 -- 453: “Optical flash of GRB 990123: constraints on the physical parameters of the reverse shock”[23] Huang Y.F., Cheng K.S., 2003, MNRAS, 341, 263 -- 269: “Gamma-ray bursts: optical afterglows in the deep Newtonian phase” [24] Fu H., Huang Y.F., 2003, Chin. J. Astron. Astrophys., 3, 535 -- 542: “Strange stars: can their crust reach the neutron dirp density?” [25] Ma H.T., Huang Y.F., Dai Z.G., Lu T., 2003, Chin. J. Astron. Astrophys., 3, 225 -- 234: “Cylindrical jet -- wind interaction model of gamma-ray burst afterglows”[26] Wu X.F., Dai Z.G., Huang Y.F., Lu T., 2003, MNRAS, 342, 1131 -- 1138: “Optical flashes and very early afterglows in wind environments”[27] Huang Y.F., Dai Z.G., Lu T., Cheng K.S., Wu X.F., 2003, ApJ, 594, 919 -- 923: “Gamma-ray bursts from neutron star kicks”[28] Liang S.L., Dai Z.G., Huang Y.F., Lu T., 2003, Chin. J. Astron. Astrophys., 3, 526 -- 534: “Extinction of beamed gamma-ray burst afterglows in a dense circumstellar cloud”[29] Huang Y.F., Wu X.F., Dai Z.G., Ma H.T., Lu T., 2004, ApJ, 605, 300 -- 306: “Rebrightening of XRF 030723: further evidence for a two-component jet in gamma-ray burst” [30] Wu X.F., Dai Z.G., Huang Y.F., Lu T., 2003, IAU Symposium, 214, 343 -- 344: “Optical flash and radio flare in wind environment” [31] Huang Y.F., Lu T., Dai Z.G., Cheng K.S., 2003, IAU Symposium, 214, 321 -- 322: “Beaming effects in gamma-ray burst afterglows” [32] Huang Y.F., Lu T., Dai Z.G., Cheng K.S., 2003, “Beaming effects in gamma-ray bursts”, in Stellar Astrophysics – A tribute to Helmut A. Abt, eds. K. S. Cheng, K. C. Leung, T. P. Li, THE SIXTH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS, JULY 11 - 11, 2002, XI'AN, CHINA [33] Jia J.J., Huang Y.F., 2004, Chinese Astron. Astr., 28, 144 -- 153: “A numerical study of the collapse of the crust of strange stars”[34] Wu X..F., Dai Z.G., Huang Y.F., Ma H.T., 2004, Chin. J. Astron. Astrophys., 4, 455 -- 472: “Afterglow light curves of jetted gamma-ray burst ejecta in stellar winds”[35] Wu X.F., Dai Z.G., Huang Y.F., Lu T., 2005, ApJ, 619, 968 -- 982: “Analytical light curves in the realistic model for gamma-ray burst afterglows” [36] Wu X.F., Dai Z.G., Huang Y.F., Lu T., 2005, MNRAS, 357, 1197 -- 1204: “Gamma-ray bursts: polarization of afterglows from two-component jets”[37] Tam P.H., Pun C.S.J., Huang Y.F., Cheng K.S., 2005, New Astronomy, 10, 535 -- 544: “Early re-brightenings in GRB afterglows as signatures of low-to-high density boundary” [38] Dai Z.G., Wu X.F., Wang X.Y., Huang Y.F., Zhang B., 2005, ApJ, 629, L81 -- L84: “A Two-Component Explosion Model for the Giant Flare and Radio Afterglow from SGR1806-20” [39] Huang Y.F., Cheng K.S., Gao T.T., 2006, ApJ, 637, 873 -- 879: “Modeling the Optical Afterglow of GRB 030329”[40] Lu Y., Cheng K.S., Huang Y.F., 2006, ApJ, 641, 288 -- 292: “Capture of a Red Giant by the Black Hole Sagittarius A* as a Possible Origin for the TeV Gamma Rays from the Galactic Center” [41] Gao T. T., Huang Y. F., 2006, Chin. J. Astron. Astrophys., 6, 305 -- 311: “On the Evolution of the Apparent Size of Gamma-Ray Burst Remnants” [42] Huang Y.F., Lu T., Cheng K.S., 2005, Nuovo Cimento Della Societa Italiana Di Fisica C-Geophysics and Space Physics, 28, 415 -- 418: “GRB afterglows: Deep Newtonian phase and its application” [43] Tam P.H., Cheng K.S., Wang X.Y., Huang Y.F., Pun J.C.S., 2005, Nuovo Cimento Della Societa Italiana Di Fisica C-Geophysics and Space Physics, 28, 447 -- 450: “Gamma-ray burst afterglows with cylindrical jet geometry” [44] Huang Y.F., Lu Y., Wong A.Y.L., Cheng K.S., 2007, Chin. J. Astron. Astrophys., 7, 397 -- 404: “A detailed study on the equal arrival time surface effect in gamma-ray burst afterglows” [45] Lu Y., Huang Y.F., Zheng Z., Zhang S.N., 2007, IAU Symposium, 238, 403 -- 404: “The capture of main sequence stars and giant stars by a massive black hole” [46] Huang Y. F., Cheng K. S., Lu Y., 2007, Advances in Space Research, 40, 1214 -- 1217: “Theoretical interpretation of the optical afterglow of GRB 030329” [47] Lu Y., Zheng Z., Zhang S.N., Huang Y.F., 2007, Astronomical Society of the Pacific Conference Series, 373, 692 -- 693: “On the nature of the flares from three candidate tidal disruption events” [48] Wu X.F., Dai Z.G., Wang X.Y., Huang Y.F., Feng L.L., Lu T., 2007, Advances in Space Research, 40, 1208 -- 1213: “X-ray flares from late internal and late external shocks” [49] Wong A. Y. L., Huang Y. F., Cheng K. S., 2007, A&A, 472, 93 -- 99: “Transient X-ray Emission from Normal Galactic Nuclei”[50] Yu Y., Huang Y.F., 2007, Chin. J. Astron. Astrophys., 7, 669 -- 674: “Shallow decay of X-ray afterglows in short GRBs: energy injection from a millisecond magnetar?” [51] Huang Yongfeng, Lu Tan, Cheng Kwong Sang, 2007, Progress in Natural Science, 17, 1261 -- 1270: “Nonrelativistic phase in -ray burst afterglows” [52] Huang Y.F., Lu Y., Cheng K.S., 2008, AIP conference proceedings, 968, 40 -- 42: “Equal arrival time surface effects in GRB afterglows” [53] Lu Y., Zheng Z., Huang Y.-F. and Zhang S.-N., 2008, AIP conference proceedings, 968, 378 -- 380: “Tidal Disruptions of Different Types of Stars by Massive Black Holes and Their Applications” [54] Xu M., Huang Y.F., and Kong S., 2008, Chin. J. Astron. Astrophys., 8, 411 -- 420: “Ring-Shaped Jets in Gamma-ray Bursts” [55] Chen L., Liu D.B., Huang Y.F., and You J.H., 2008, ApJ, 680, 539 -- 544: “Does the prompt -ray emission of gamma-ray bursts arise from resonant inverse compton scattering?”[56] Jia J.J., Huang Y.F., Cheng K.S., 2008, ApJ, 677, 488 -- 494: “A morphological approach to the pulsed emission from soft gamma repeaters”[57] Lu Y., Huang Y.F., Zhang S.N., 2008, ApJ, 684, 1330 -- 1335: “A tidal disruption model for the gamma-ray burst of GRB 060614” [58] Huang Y. F., Lu T., 2008, AIP Conference Proceedings, 1065, 165 -- 168: “GRB Afterglows in the Nonrelativistic Phase” [59] Kong S.W., Huang Y.F., 2008, AIP Conference Proceedings, 1065, 173 – 176: “Modeling the Radio and Optical/NIR Afterglows of GRB 980703: a Numerical Study” [60] Xu M., Huang Y.F., Kong S.W., 2008, AIP Conference Proceedings, 1065, 177 – 180: “Afterglows from Ring-Shaped Jet” [61] Lu Y., Huang Y.F., Zhang S.N., 2008, AIP Conference Proceedings, 1065, 285 – 288: “The Origin of the Gamma-Ray Burst of GRB 060614” [62] Liu D.B., Huang Y.F., You J.H., Chen L., 2008, AIP Conference Proceedings, 1065, 211 – 217: “Does the Prompt Gamma-Ray Emission of GRB Arise from RICS?” [63] Kong S.W., Huang Y.F., Cheng K.S., LuT. 2009, Science in China Series G, 52(12): 2047-2053: “Modeling the Radio and Optical/NIR Afterglows of GRB 980703: a Numerical Study” [64] Wang X., Huang Y.F., Kong S.-W., 2009, A&A, 505, 1213-1219: “On the afterglow from the receding jet of gamma-ray bursts” [65] Xu M., Huang Y.F., 2010, Sci. China-Phys. Mech. Astron, 53(Suppl.1), 91-93: “A model for the optical flares from the Galactic transient SWIFT J195509+261406” [66] Wang X., Huang Y.F., Kong S.W., 2010, Sci. China-Phys. Mech. Astron,2010, 53(Suppl.1), 259-261: “Constraint on the counter-jet emission in gamma-ray burst afterglows from GRB 980703” [67] Kong S.W., Huang Y.F., 2010, Sci. China-Phys. Mech. Astron,2010, 53(Suppl.1), 94-97: “Afterglow from GRB 070610/Swift J195509.6+261406: an explanation using the fireball model” [68] Xu M., Huang Y.F., Lu T., 2009, Research in Astron. Astrophys, 9, 1317–1323: “Long-term Continuous Energy Injection in the Afterglow of GRB 060729” [69] Cheng K.S., Harko T., Huang Y.F., Lin L.M., Suen W.M., Tian X.L., 2009, Journal of Cosmology and Astroparticle Physics, 9, Art. No. 007: “Relativistic Mass Ejecta from Phase-transition-induced Collapse of Neutron Stars” [70] Kong S.W., Wong A.Y.L., Huang Y.F., Cheng K.S., 2010, MNRAS, 402, 409 – 416: “Variation of microphysics in wind bubbles: an alternative mechanism for explaining the rebrightenings in Gamma-ray burst afterglows” [71] Deng Wei, Huang Y.F., Kong S.W., 2010, RAA, 10, 1119–1126: “Measuring the beaming angle of GRB 030329 by fitting the rebrightenings in its multiband afterglow”[72] Xu M., Huang Y. F., 2010, A&A, 523, A5(5pp): “Early Rebrightenings of X-ray Afterglows from Ring-Shaped GRB Jets” (DOI: 10.1051/0004-6361/201014352)[73] Xu M., Nagataki S., Huang Y. F., Lee, S. H., 2012, ApJ, 746, 49(6pp): “Failed Gamma-Ray Bursts: Thermal Ultraviolet/Soft X-Ray Emission Accompanied by Peculiar Afterglows” [74] Kong S.W., Yu Y.W., Huang Y.F., Cheng K.S., 2011, MNRAS, 416, 1067-1076: “Modeling the multiwavelength light curves of PSR B1259-63/SS 2883”[75] Xu M., Huang Y.F., 2012, A&A, 538, A134(5pp): “New three-parameter correlation for gamma-ray bursts with a plateau phase in the afterglow” [76] Xu M., Nagataki S., Huang Y.F., 2011, ApJ, ApJ, 735, 3(5pp): “An Off-Axis Relativistic Jet Model for the Type Ic supernova SN 2007gr”[77] Gong Biping, Kong S.W., Xue F., Li Yaping, Huang Y.F., 2011, MNRAS, 418, 2451-2458: “Non-ballistic superluminal motion in the plane of the sky - II” [78] Shi Ke, Huang Yong-Feng and Lu Tan, 2011, RAA, 11, 1403-1412: “The effects of parametrization of the dark energy equation of state” [79] Huang Y.F., Cheng K.S., Dai Z.G., Lu T., 2004, AIP Conference Proceedings, 727, 475-478: “GRB afterglows in the deep Newtonian phase” [80] Kong S. W., Cheng K. S., Huang Y. F., 2012, ApJ, 753, 127(9pp): “Modelling the multiwavelength light curves of PSR B1259-63/LS 2883 - II. The effects of anisotropic pulsar wind and Doppler boosting” [81] Zhang Z. B., Chen D. Y., and Huang Y. F., 2012, ApJ, 755, 55: “Correlation between Peak Energy and Peak Luminosity in Short Gamma-Ray Bursts”[82] Shi K., Huang Y.F., and Lu T., 2012, MNRAS, 426, 2452-2462: “A comprehensive comparison of cosmological models from the latest observational data” [83] Shi K., Huang Y.F., and Lu T., 2012, Physics Letters B, 717, 299-306: “Constraining dark energy using observational growth rate data”[84] Geng J.J. and Huang Y.F., 2013, ApJ, 764, 75 (9 pp), “On the Correlation of Low-energy Spectral Indices and Redshifts of Gamma-ray Bursts” [85] Wang Xin, Meng Xiao-Lei, Zhang Tong-Jie, Shan HuanYuan, Gong Yan, Tao Charling, Chen Xuelei, Huang Y. F., 2012, JCAP, 11, 018: “Observational constraints on cosmic neutrinos and dark energy revisited” [86] Zhang Zhibin, Huang Y. F., Liu, Hongchao, 2013, IAU Symposium, 290, 361-363: “On the Reclassification of Short GRBs” [87] Yu Yongbo, Huang Y. F., 2013, RAA, 13, 662–670: “A two-step energy injection explanation for the rebrightenings of the multi-band afterglow of GRB 081029” [88] Huang Y. F., Geng J. J., 2014, ApJ, 782, L20(4pp): “Anti-glitch induced by collision of a solid body with the magnetar 1E 2259+586” [89] Geng J. J., Wu X. F., Huang Y. F., Yu Y. B., 2013, ApJ, 779, 28(9pp): “Delayed Energy Injection Model For Gamma-Ray Burst Afterglows” [90] Wang X., Meng X. L., Huang Y. F., Zhang T. J., 2013, RAA, 13, 1013-1024: “Testing X-ray Measurements of Galaxy Cluster Gas Mass Fraction Using the Cosmic Distance-Duality Relation” [91] Hou S. J., Geng J. J., Wang K., Wu X. F., Huang Y. F., Dai Z. G., Lu J. F., 2014, ApJ, 785, 113: “The origin of the plateau and late rebrightening in the afterglow of GRB 120326A”[92] Zhang Z. B., Kong S. W., Huang Y. F., Li D., Li L. B., 2015, RAA, 15, 237–251: “Detecting Radio Afterglows of Gamma-Ray Bursts with FAST” [93] Geng J. J., Wu X. F., Li L., Huang Y. F., Dai Z. G., 2014, ApJ, 792, 31(10pp): “Revisiting the Emission from Relativistic Blast Waves in a Density-Jump Medium” [94] Yu Y. B., Wu X. F., Huang Y. F., Coward D. M., Stratta G., Gendre B., Howell E. J., 2015, MNRAS, 446, 3642 -- 3650: “Fall back accretion and energy injections in gamma-ray bursts” [95] Geng J. J., Huang Y. F., Lu T., 2015, ApJ, 804, 21(5pp): “Coalescence of strange-quark planets with strange stars: a new kind of source for gravitational wave bursts” [96] Zhang S.N. et al., 2014, Proceedings of the SPIE, Volume 9144, id. 91440X 9 pp: “The high energy cosmic-radiation detection (HERD) facility onboard China's future Space Station”, SPIE Astronomical Telescopes + Instrumentation meeting on June 23 in Montreal, Canada, [97] Li L., Wu X. F., Huang Y. F., et al., 2015, ApJ, 805, 13: “A Correlated Study of Optical and X-ray Afterglows of GRBs” [98] Yu Y. B., Huang Y. F., Wu X. F., Xu M., Geng J. J., 2015, ApJ, 805, 88(6pp): “Signature of a spin-up magnetar from multi-band afterglow rebrightening of GRB 100814A” [99] Li L. B., Zhang Z. B., Huang Y. F., Wu X. F., Kong S. W., Li D., Chang H. Y., Choi C. S., 2015, MNRAS, 451, 1815–1823: “Radio afterglows and host galaxies of gamma-ray bursts”, [100] Huang Y. F., Geng J. J., Zhang, Z. B., 2015, Chinese Astronomy & Astrophysics, published: “Collision-induced glitch/anti-glitches” [101] Xu M., Huang Y. F., 2015, RAA, 15, 986–992: “Effect of rapid evolution of magnetic tilt angle on newborn magnetar’s dipole radiation” [102] Zheng Xing-wu, Huang Yong-feng, 1996, ChA&A, 20, 437: “The density and magnetic field of the dense cores of the molecular cloud L 1630” [103] Tam P. H., Cheng K. S., Pun C. S. J., Huang Y. F., 2004, AAS, 204, 6313: \中国天文学会会员,国际天文学联合会会员 相关热点
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