Zobrazeno 1 - 10
of 24 014
pro vyhledávání: '"You, Y"'
Autor:
Xiao, Y. X., Xu, Y. J., Ge, M. Y., Lu, F. J., Zhang, S. N., Zhang, S., Tao, L., Qu, J. L., Wang, P. J., Kong, L. D., Tuo, Y. L., You, Y., Zhao, S. J., Peng, J. Q., Du, Y. F., Zhang, Y. H., Ye, W. T.
We report the phase-resolved spectral results of the first Galactic Pulsating Ultra-Luminous X-ray source (PULX) Swift J0243.6+6124, modeling at its 2017-2018 outburst peak using data collected by the Hard X-ray Modulation Telescope (Insight-HXMT). T
Externí odkaz:
http://arxiv.org/abs/2401.15992
Publikováno v:
Journal of Hepatocellular Carcinoma, Vol Volume 11, Pp 1031-1048 (2024)
Shuxiu Xiao,1,* Lili Lu,1,* Zhiyuan Lin,2,* Xinming Ye,3 Sheng Su,3 Chenlu Zhang,4 Yang You,4 Wei Li,4 Xiaowu Huang,3 Weizhong Wu,5 Yuhong Zhou1,4 1Clinical Center for Biotherapy, Zhongshan Hospital, Fudan University, Shanghai, 200032, Pe
Externí odkaz:
https://doaj.org/article/555e7428275141e7a6080c30d554be09
Publikováno v:
Therapeutics and Clinical Risk Management, Vol Volume 20, Pp 297-311 (2024)
Zihui Yuan,* Chao Du,* Yun You,* Jian Wang Department of Vascular Surgery, Union Hospital, Tongji Medical College, Huazhong University of Science and Technology, Wuhan, People’s Republic of China*These authors contributed equally to
Externí odkaz:
https://doaj.org/article/2e530ad253c14e1aa2f7c2a48d07ae4f
Autor:
Hou, X., You, Y., Ji, L., Soria, R., Zhang, S. N., Ge, M. Y., Tao, L., Zhang, S., Feng, H., Zhou, M., Tuo, Y. L., Song, L. M., Wang, J. C.
Pulsating ultraluminous X-ray sources (PULXs) are accreting pulsars with apparent X-ray luminosity exceeding $10^{39}\, \rm erg\ s^{-1}$. We perform Monte-Carlo simulations to investigate whether high collimation effect (or strong beaming effect) is
Externí odkaz:
http://arxiv.org/abs/2211.08021
Autor:
Hou, X., Ge, M. Y., Ji, L., Zhang, S. N., You, Y., Tao, L., Zhang, S., Soria, R., Feng, H., Zhou, M., Tuo, Y. L., Song, L. M., Wang, J. C.
We present detailed timing and spectral analyses of the transient X-ray pulsar RX J0209.6$-$7427 in the Small Magellanic Cloud during its 2019 giant outburst. With a better known distance than most galactic X-ray pulsars, its peak luminosity is deter
Externí odkaz:
http://arxiv.org/abs/2208.14785
Publikováno v:
Journal of Mining and Metallurgy. Section B: Metallurgy, Vol 60, Iss 1, Pp 127-137 (2024)
Understanding reaction kinetics can provide valuable information for the design and optimization of a reaction process. In this study, the reduction degree and carbonitriding ratio of TiO2 in the CH4-H2-N2 system were investigated to understand the k
Externí odkaz:
https://doaj.org/article/449309f340304daca7d7881682db3ab9
Publikováno v:
International Journal of General Medicine, Vol Volume 16, Pp 5947-5953 (2023)
Zhimei Zhao,1,* Xiang Han,1,* Yunhong You,1 Jiankang Zhang,2 Keke Nie,1 Youxin Ji1 1Department of Oncology, Affiliated Qingdao Central Hospital of Qingdao University, Qingdao Cancer Hospital, Qingdao City, People’s Republic of China; 2Depar
Externí odkaz:
https://doaj.org/article/5778112270d84ccabf78b50a48e3a2e7
Autor:
Robin, P., Emmerich, T., Ismail, A., Niguès, A., You, Y., Nam, G. -H., Keerthi, A., Siria, A., Geim, A. K., Radha, B., Bocquet, L.
Publikováno v:
Science 379, 161-167 (2023)
Fine-tuned ion transport across nanoscale pores is key to many biological processes such as neurotransmission. Recent advances have enabled the confinement of water and ions to two dimensions, unveiling transport properties unreachable at larger scal
Externí odkaz:
http://arxiv.org/abs/2205.07653
The pursuit of knowledge in particle physics requires constant learning. As new tools become available, new theories are developed, and physicists search for new answers with ever-evolving methods. However, it is the case that formal educational syst
Externí odkaz:
http://arxiv.org/abs/2204.08983
Autor:
Cai, C., Xiong, S. L., Li, C. K., Liu, C. Z., Zhang, S. N., Li, X. B., Song, L. M., Li, B., Xiao, S., Yi, Q. B., Zhu, Y., Zheng, Y. G., Chen, W., Luo, Q., Huang, Y., Song, X. Y., Zhao, H. S., Zhao, Y., Zhang, Z., Bu, Q. C., Cao, X. L., Chang, Z., Chen, L., Chen, T. X., Chen, Y. B., Chen, Y., Chen, Y. P., Cui, W. W., Du, Y. Y., Gao, G. H., Gao, H., Ge, M. Y., Gu, Y. D., Guan, J., Guo, C. C., Han, D. W., Huo, J., Jia, S. M., Jiang, W. C., Jin, J., Kong, L. D., Li, G., Li, T. P., Li, W., Li, X., Li, X. F., Li, Z. W., Liang, X. H., Liao, J. Y., Liu, B. S., Liu, H. W., Liu, H. X., Liu, X. J., Lu, F. J., Lu, X. F., Luo, T., Ma, R. C., Ma, X., Meng, B., Nang, Y., Nie, J. Y., Ou, G., Qu, J. L., Ren, X. Q., Sai, N., Sun, L., Tan, Y., Tao, L., Tuo, Y. L., Wang, C., Wang, L. J., Wang, P. J., Wang, W. S., Wang, Y. S., Wen, X. Y., Wu, B. B., Wu, B. Y., Wu, M., Xiao, G. C., Xu, Y. P., Yang, R. J., Yang, S., Yang, Y. J., Yang, Y. R., Yang, X. J., Yin, Q. Q., You, Y., Zhang, F., Zhang, H. M., Zhang, J., Zhang, P., Zhang, S., Zhang, W. C., Zhang, W., Zhang, Y. F., Zhang, Y. H., Zhao, X. F., Zheng, S. J., Zhou, D. K.
The High Energy X-ray telescope (HE) on-board the Hard X-ray Modulation Telescope (\textit{Insight}-HXMT) can serve as a wide Field of View (FOV) gamma-ray monitor with high time resolution ($\mu$s) and large effective area (up to thousands cm$^2$).
Externí odkaz:
http://arxiv.org/abs/2109.12270