Zobrazeno 1 - 10
of 645
pro vyhledávání: '"J. A. Yao"'
Autor:
X. L. Wu, C. Zheng, M. Xu, A. J. Zheng, L. L. Zhu, P. X. Li, J. H. Yao, M. Wang, J. H. Wang, W. H. Xu
Publikováno v:
Metalurgija, Vol 63, Iss 3-4, Pp 439-442 (2024)
In this study, a Finite Element Computational (FEC) model for automotive bellows exhaust pipes is established, and the impact of displacement loads on their fatigue life is investigated. The relationships between various structural parameters of the
Externí odkaz:
https://doaj.org/article/6f1313163dc94ee894f694ca64cbb233
Autor:
D. Zhao, N. Wang, J. P. Yuan, D. Li, P. Wang, M. Y. Xue, W. W. Zhu, C. C. Miao, W. M. Yan, J. B. Wang, J. M. Yao, Q. D. Wu, S. Q. Wang, S. N. Sun, F. F. Kou, Y. T. Chen, S. J. Dang, Y. Feng, Z. J. Liu, X. L. Miao, L. Q. Meng, M. Yuan, C. H. Niu, J. R. Niu, L. Qian, S. Wang, X. Y. Xie, Y. F. Xiao, Y. L. Yue, S. P. You, X. H. Yu, R. S. Zhao, R. Yuen, X. Zhou, L. Zhang, Y. B. Wang, J. F. Wu, Z. Y. Gan, Z. Y. Sun, C. J. Wang
Publikováno v:
The Astrophysical Journal Letters, Vol 974, Iss 2, p L39 (2024)
Externí odkaz:
https://doaj.org/article/8acf4a1765a04ef3ba77188e72e5b2a0
Autor:
D. Zhao, N. Wang, J. P. Yuan, D. Li, P. Wang, M. Y. Xue, W. W. Zhu, C. C. Miao, W. M. Yan, J. B. Wang, J. M. Yao, Q. D. Wu, S. Q. Wang, S. N. Sun, F. F. Kou, Y. T. Chen, S. J. Dang, Y. Feng, Z. J. Liu, X. L. Miao, L. Q. Meng, M. Yuan, C. H. Niu, J. R. Niu, L. Qian, S. Wang, X. Y. Xie, Y. F. Xiao, Y. L. Yue, S. P. You, X. H. Yu, R. S. Zhao, R. Yuen, X. Zhou, L. Zhang, Y. B. Wang, J. F. Wu, Z. Y. Gan, Z. Y. Sun, C. J. Wang
Publikováno v:
The Astrophysical Journal Letters, Vol 964, Iss 1, p L7 (2024)
We report the timing analysis of PSR J1846−0513, a pulsar discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in Commensal Radio Astronomy FAST Survey. The pulsar possesses a spin period of 23.36 ms and a spin-down rate (
Externí odkaz:
https://doaj.org/article/25d8511d1b45400ca7fe662b28d2fb88
Autor:
Erin Jay G. Feliciano, Frances Dominique V. Ho, Kaisin Yee, Joseph A. Paguio, Michelle Ann B. Eala, Janine Patricia G. Robredo, Kenrick Ng, Jasmine Lim, Khin Thuzar Pyone, Catherine A. Peralta, Jerickson Abbie Flores, J. Seth Yao, Patricia Mae G. Santos, Christian Daniel U. Ang, Gideon Lasco, Jeffrey Shi Kai Chan, Gary Tse, Enrico D. Tangco, T. Peter Kingham, Imjai Chitapanarux, Nirmala Bhoo-Pathy, Gerardo D. Legaspi, Edward Christopher Dee
Publikováno v:
The Lancet Regional Health. Western Pacific, Vol 41, Iss , Pp 100971- (2023)
Externí odkaz:
https://doaj.org/article/5718ec76610c47109cabc9ba8464ef2e
Autor:
D. Zhao, J. P. Yuan, N. Wang, D. Li, P. Wang, M. Y. Xue, W. W. Zhu, C. C. Miao, W. M. Yan, J. B. Wang, J. M. Yao, Q. D. Wu, S. Q. Wang, S. N. Sun, F. F. Kou, Y. T. Chen, S. J. Dang, Y. Feng, Z. J. Liu, X. L. Miao, L. Q. Meng, M. Yuan, C. H. Niu, J. R. Niu, L. Qian, S. Wang, X. Y. Xie, Y. F. Xiao, Y. L. Yue, S. P. You, X. H. Yu, R. S. Zhao, R. Yuen, X. Zhou, L. Zhang, M. Xie, Y. X. Li, Y. B. Wang, Z. K. Luo, Z. Y. Gan, Z. Y. Sun, M. M. Chi, C. J. Wang
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 1, p 88 (2024)
We present phase-connected timing ephemerides, polarization pulse profiles, and Faraday rotation measurements of 12 pulsars discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in the Commensal Radio Astronomy FAST Survey. T
Externí odkaz:
https://doaj.org/article/284aaa634b0240e7a19ce2b41f3a1b5c
Autor:
Q. D. Wu, N. Wang, J. P. Yuan, D. Li, P. Wang, M. Y. Xue, W. W. Zhu, C. C. Miao, W. M. Yan, J. B. Wang, J. M. Yao, S. Q. Wang, S. N. Sun, F. F. Kou, D. Zhao, Y. T. Chen, S. J. Dang, Y. Feng, Z. J. Liu, X. L. Miao, L. Q. Meng, M. Yuan, C. H. Niu, J. R. Niu, L. Qian, S. Wang, X. Y. Xie, Y. F. Xiao, Y. L. Yue, S. P. You, X. H. Yu, R. S. Zhao, R. Yuen, X. Zhou, L. Zhang
Publikováno v:
The Astrophysical Journal Letters, Vol 958, Iss 1, p L17 (2023)
PSR J2150+3427 is a 0.654 s pulsar discovered by the Commensal Radio Astronomy FAST Survey. From the follow-up observations, we find that the pulsar is in a highly eccentric orbit ( e = 0.601) with an orbital period of 10.592 days and a projected sem
Externí odkaz:
https://doaj.org/article/768260cedc594d0c9cc8fea7c6df84af
Autor:
S. Q. Wang, J. B. Wang, D. Z. Li, J. M. Yao, R. N. Manchester, G. Hobbs, N. Wang, S. Dai, H. Xu, R. Luo, Y. Feng, W. Y. Wang, D. Li, Y. W. Yu, Z. X. Du, C. H. Niu, S. B. Zhang, C. M. Zhang
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 1, p 36 (2023)
Black widows are millisecond pulsars ablating their companions. The material blown from the companion blocks the radio emission, resulting in radio eclipses. The properties of the eclipse medium are poorly understood. Here, we present direct evidence
Externí odkaz:
https://doaj.org/article/05f9d8a94b9e4cf7ad87a15b2944f1ca
Autor:
Q D Wu, J P Yuan, N Wang, D Li, P Wang, M Y Xue, W W Zhu, C C Miao, W M Yan, J B Wang, J M Yao, S Q Wang, S N Sun, F F Kou, Z Y Tu, J T Xie, Z C Pan, D Zhao, Y T Chen, S J Dang, Y Feng, Z J Liu, X L Miao, L Q Meng, M Yuan, C H Niu, J R Niu, L Qian, S Wang, X Y Xie, Y F Xiao, Y L Yue, S P You, X H Yu, R S Zhao, L Zhang, R Yuen, Z G Wen, H M Tedila
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:5152-5164
The follow-up timing observations were carried out for 24 pulsars discovered with the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in Commensal Radio Astronomy FAST Survey. We report their phase-connected timing ephemeris, polarizatio
Publikováno v:
Plant Biology. 25:334-342
Autor:
C C Miao, W W Zhu, D Li, P C C Freire, J R Niu, P Wang, J P Yuan, M Y Xue, A D Cameron, D J Champion, M Cruces, Y T Chen, M M Chi, X F Cheng, S J Dang, M F Ding, Y Feng, Z Y Gan, G Hobbs, M Kramer, Z J Liu, Y X Li, Z K Luo, X L Miao, L Q Meng, C H Niu, Z C Pan, L Qian, Z Y Sun, N Wang, S Q Wang, J B Wang, Q D Wu, Y B Wang, C J Wang, H F Wang, S Wang, X Y Xie, M Xie, Y F Xiao, M Yuan, Y L Yue, J M Yao, W M Yan, S P You, X H Yu, D Zhao, R S Zhao, L Zhang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 518:1672-1682
We report the phase-connected timing ephemeris, polarization pulse profiles, Faraday rotation measurements, and Rotating-Vector-Model (RVM) fitting results of 12 millisecond pulsars (MSPs) discovered with the Five-hundred-meter Aperture Spherical rad