المؤلفون: Shang, Lun-Hua, Lu, Ji-Guang, Du, Yuan-Jie, Hao, Long-Fei, Li, Di, Lee, Ke-Jia, Li, Bin, Li, Li-Xin, Qiao, Guo-Jun, Shen, Zhi-Qiang, Wang, De-Hua, Wang, Min, Wu, Xin-Ji, Wu, Ya-Jun, Xu, Ren-Xin, Yue, You-Ling, Yan, Zhen, Zhi, Qi-Jun, Zhao, Rong-Bing, Zhao, Ru-Shuang

المساهمون: Shang, LH, Zhi, QJ (reprint author), Guizhou Normal Univ, Sch Phys & Elect Sci, 116 Baoshan Rd, Guiyang 550001, Peoples R China., Shang, LH (reprint author), Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China., Qiao, GJ (reprint author), Peking Univ, Sch Phys, 5 Yiheyuan Rd, Beijing 100871, Peoples R China., Zhi, QJ (reprint author), NAOC GZNU, Ctr Astron Res & Educ, 116 Baoshan Rd, Guiyang 550001, Peoples R China., Guizhou Normal Univ, Sch Phys & Elect Sci, 116 Baoshan Rd, Guiyang 550001, Peoples R China., Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China., Peking Univ, Sch Phys, 5 Yiheyuan Rd, Beijing 100871, Peoples R China., Peking Univ, State Key Lab Nucl Sci & Technol, 5 Yiheyuan Rd, Beijing 100871, Peoples R China., Qian Xuesen Lab Space Technol, 104 Youyi Rd, Beijing 100094, Peoples R China., Chinese Acad Sci, Yunnan Astron Observ, 396 Yangfangwang, Guandu Dist 650011, Kunming, Peoples R China., Peking Univ, Kavil Inst Astron & Astrophys, 5 Yiheyuan Rd, Beijing 100871, Peoples R China., Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China., Chinese Acad Sci, Key Lab Radio Astron, 80 Nandan Rd, Shanghai 200030, Peoples R China., NAOC GZNU, Ctr Astron Res & Educ, 116 Baoshan Rd, Guiyang 550001, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: radiation mechanisms: non-thermal, stars: magnetic field, stars: neutron, pulsars: individual: PSR B0329+54, pulsars: individual: PSR B1642-03, GAMMA-RAY EMISSION, MULTICOMPONENT GAUSSIAN FITS, INNER ANNULAR GAP, RADIO PULSARS, WIDTH STATISTICS, GEOMETRICAL ANALYSIS, CURVATURE RADIATION, INTEGRATED PROFILES, MILLISECOND PULSARS, HIGH-FREQUENCIES

Relation: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY.2017,468(4),4389-4398.; 1906713; http://hdl.handle.net/20.500.11897/472549; WOS:000402819700049

الاتاحة: https://hdl.handle.net/20.500.11897/472549
https://doi.org/10.1093/mnras/stx815

المؤلفون: Shang, Lun-Hua, Lu, Ji-Guang, Du, Yuan-Jie, Hao LF(郝龙飞), Li, Di, Lee, Ke-Jia, Li, Bin, Li, Li-Xin, Guo, Jun-Qiao, Shen, Zhi-Qiang, Wang, De-Hua, Wang M(汪敏), Wu, Xin-Ji, Wu, Ya-Jun, Xu, Ren-Xin, Yue, You-Ling, Yan, Zhen, Zhi, Qi-Jun, Zhao, Rong-Bing, Zhao, Ru-Shuang

مصطلحات موضوعية: Radiation Mechanisms: Non-thermal, Stars: Magnetic Field, Stars: Neutron, Pulsars: Individual: Psr b0329+54, Pulsars: Individual: Psr B1642-03, 天文学, 天文学::射电天文学, 理学, 理学::天文学, Astronomy & Astrophysics, GAMMA-RAY EMISSION, MULTICOMPONENT GAUSSIAN FITS, INNER ANNULAR GAP, RADIO PULSARS, WIDTH STATISTICS, GEOMETRICAL ANALYSIS, CURVATURE RADIATION, INTEGRATED PROFILES, MILLISECOND PULSARS, HIGH-FREQUENCIES, Radiation, 657.2 Extraterrestrial Physics and Stellar Phenomena - 932.1 High Energy Physics, Science & Technology, Physical Sciences

Relation: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY; http://ir.ynao.ac.cn/handle/114a53/10089

الاتاحة: http://ir.ynao.ac.cn/handle/114a53/10089
https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stx815
https://doi.org/10.1093/mnras/stx815

المؤلفون: Dai, S., Hobbs, G., Manchester, R. N., Kerr, M., Shannon, R. M., van Straten, W., Mata, A., Bailes, M., Bhat, N. D. R., Burke-Spolaor, S., Coles, W. A., Johnston, S., Keith, M. J., Levin, Y., Oslowski, S., Reardon, D., Ravi, V., Sarkissian, J. M., Tiburzi, C., Toomey, L., Wang, H. G., Wang, J.B., Wen, L., Xu, R. X., Yan, W. M., Zhu, X.J.

المساهمون: Dai, S (reprint author), Peking Univ, Sch Phys, Beijing 100871, Peoples R China., Peking Univ, Sch Phys, Beijing 100871, Peoples R China., Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China., CSIRO Astron & Space Sci, Australia Telescope Natl Facil, Epping, NSW 1710, Australia., Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia., Univ Texas Brownsville, Ctr Adv Radio Astron, Brownsville, TX 78520 USA., Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia., CALTECH, Dept Astron, Pasadena, CA 91125 USA., Univ Calif San Diego, Dept Elect & Comp Engn, La Jolla, CA 92093 USA., Univ Manchester, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England., Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia., Max Planck Inst Radioastron, D-53121 Bonn, Germany., Univ Bielefeld, Dept Phys, D-33615 Bielefeld, Germany., Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia., CSIRO Astron & Space Sci, Parkes Observ, Parkes, NSW 2870, Australia., Osservatorio Astron Cagliari, INAF, I-09047 Selargius, CA, Italy., Univ Cagliari, Dipartimento Fis, I-09042 Monserrato, CA, Italy., Guangzhou Univ, Sch Phys & Elect Engn, Guangzhou 510006, Guangdong, Peoples R China., Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China., Univ Western Australia, Sch Phys, Crawley, WA 6009, Australia., Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: polarization, radiation mechanisms: non-thermal, pulsars: general, radio continuum: general, LARGE-AREA TELESCOPE, GAMMA-RAY PULSARS, MULTICOMPONENT GAUSSIAN FITS, RADIO-EMISSION, EMPIRICAL-THEORY, TIMING ARRAY, FREQUENCY-DEPENDENCE, GEOMETRICAL ANALYSIS, ROTATION MEASURES, FARADAY-ROTATION

Relation: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY.2015,449,(3),3223-3262.; 1307128; http://hdl.handle.net/20.500.11897/419962; WOS:000355337800080

الاتاحة: https://hdl.handle.net/20.500.11897/419962
https://doi.org/10.1093/mnras/stv508

المؤلفون: Lv, M., Wang, H. G., Lee, K. J., Qiao, G. J., Xu, R. X.

المساهمون: Lv, M (reprint author), Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China., Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China., Max Planck Inst Radio Astron, D-53121 Bonn, Germany., Peking Univ, Dept Astron, Beijing 100871, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: methods: data analysis, pulsars: general, radiation mechanisms: non-thermal, MULTICOMPONENT GAUSSIAN FITS, EMPIRICAL-THEORY, GEOMETRICAL ANALYSIS, EMISSION REGION, PAIR CASCADES, CORE EMISSION, ICS MODEL, PROFILES, POLARIZATION, FREQUENCIES

Relation: ASTROPHYSICAL JOURNAL.2011,741,(1).; 898964; http://hdl.handle.net/20.500.11897/394303; WOS:000296769000002

الاتاحة: https://hdl.handle.net/20.500.11897/394303
https://doi.org/10.1088/0004-637X/741/1/2

المؤلفون: Zhang, H., Qiao, G. J., Han, J. L., Lee, K. J., Wang, H. G.

المساهمون: Zhang, H (reprint author), Chinese Acad Sci, Natl Astron Observ, Jia 20 Datun Rd, Beijing 100012, Peoples R China., Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China., Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Guangzhou Univ, Ctr Astrophys, Guangzhou 510400, Peoples R China., Chinese Acad Sci, Natl Astron Observ, Jia 20 Datun Rd, Beijing 100012, Peoples R China.

المصدر: SCI ; EI

مصطلحات موضوعية: stars : pulsars individual : PSR B2111+46, radiation mechanisms : non-thermal, MULTICOMPONENT GAUSSIAN FITS, PULSAR EMISSION, GEOMETRICAL ANALYSIS, EMPIRICAL-THEORY, ICS MODEL, ALTITUDES, BEAMS, MAGNETOSPHERES, FREQUENCIES, RADIATION

Relation: ASTRONOMY & ASTROPHYSICS.2007,465,(2),525-531.; 977633; http://hdl.handle.net/20.500.11897/398479; WOS:000245107900019

الاتاحة: https://hdl.handle.net/20.500.11897/398479
https://doi.org/10.1051/0004-6361:20066550

المؤلفون: Xu, XB, Wu, XJ

المساهمون: Xu, XB (reprint author), Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Peking Univ, Dept Astron, Beijing 100871, Peoples R China., Chinese Acad Sci, Urumqi Astron Observat, Urumqi 830011, Peoples R China., CAS, PKU Joint Beijing Astrophys Ctr, Beijing 100871, Peoples R China.

المصدر: SCI

مصطلحات موضوعية: pulsars, component decomposition, emission region, MULTICOMPONENT GAUSSIAN FITS, CONAL EMISSION REGION, EMPIRICAL-THEORY, GEOMETRICAL ANALYSIS, PROFILE, FREQUENCIES

Relation: SCIENCE IN CHINA SERIES G-PHYSICS MECHANICS & ASTRONOMY.2003,46,(1),104-112.; 1012055; http://hdl.handle.net/20.500.11897/298391; WOS:000181438600015

الاتاحة: https://hdl.handle.net/20.500.11897/298391
https://doi.org/10.1360/03yg9015