Zobrazeno 1 - 10
of 9 718
pro vyhledávání: '"Hao, C."'
Unraveling the internal kinematics of open clusters is crucial for understanding their formation and evolution. However, there is a dearth of research on this topic, primarily due to the lack of high-quality kinematic data. Using the exquisite-precis
Externí odkaz:
http://arxiv.org/abs/2402.12160
Autor:
Kvapil, J., Borca-Tasciuc, G., Bossi, H., Chen, K., Chen, Y., Morales, Y. Corrales, Da Costa, H., Da Silva, C., Dean, C., Durham, J., Fu, S., Hao, C., Harris, P., Hen, O., Jheng, H., Lee, Y., Li, P., Li, X., Lin, Y., Liu, M. X., Olvera, A., Purschke, M. L., Rigatti, M., Roland, G., Schambach, J., Shi, Z., Tran, N., Wuerfel, N., Xu, B., Yu, D., Zhang, H.
The RHIC interaction rate at sPHENIX will reach around 3 MHz in pp collisions and requires the detector readout to reject events by a factor of over 200 to fit the DAQ bandwidth of 15 kHz. Some critical measurements, such as heavy flavor production i
Externí odkaz:
http://arxiv.org/abs/2312.15104
Publikováno v:
International Journal of COPD, Vol Volume 19, Pp 2001-2010 (2024)
Jun Guo,1 Jie Yang,2 Jinghua Wang,3 Wei Liu,1 Yingjie Kang,4 Zhi Li,1 Chen Hao,1 Shuai Qi1 1General Surgery, Bethune International Peace Hospital, Shijiazhuang, People’s Republic of China; 2Cadre Ward, Bethune International Peace Hospital, Shijiazh
Externí odkaz:
https://doaj.org/article/157ac53259bd4de6bbf791cb52f434ad
We systematically compare the temporal and spectral properties of 53 Supernova (SN)-associated and 15 Kilonova (KN)-associated Gamma-Ray Bursts (GRBs). We find that the spectral parameters of both types GRBs are identically and lognormally distribute
Externí odkaz:
http://arxiv.org/abs/2306.03365
Open clusters (OCs) are infrequent survivors of embedded clusters gestated in molecular clouds. Up to now, little is known about the initial conditions for the formation of OCs. Here, we studied this issue using high-precision astrometric parameters
Externí odkaz:
http://arxiv.org/abs/2305.04415
In spite of much work, the overall spiral structure morphology of the Milky Way remains somewhat uncertain. In the last two decades, accurate distance measurements have provided us with an opportunity to solve this issue. Using the precise locations
Externí odkaz:
http://arxiv.org/abs/2304.10690
Publikováno v:
Journal of Multidisciplinary Healthcare, Vol Volume 17, Pp 3917-3929 (2024)
Yan Wang,1 Lihua Liang,2,* Ran Li,2,* Yihua Wang,3 Changfu Hao1 1Department of Child and Adolescent Health, School of Public Health, Zhengzhou University, Zhengzhou, Henan, People’s Republic of China; 2Primary and Secondary School Health Ce
Externí odkaz:
https://doaj.org/article/602c9c62568047b6935684b593d13fd9
Publikováno v:
Cancer Management and Research, Vol Volume 16, Pp 1021-1030 (2024)
Guo-Qiang Xue, Cheng-Peng Li, Ang Lv, Jian-Hui Wu, Xiu-Yun Tian, Hui Qiu, Chunyi Hao Key Laboratory of Carcinogenesis and Translational Research (Ministry of Education/Beijing), Department of Hepato-Pancreato-Biliary Surgery/Sarcoma Center, Peking Un
Externí odkaz:
https://doaj.org/article/d0b5342151ea4ab6bfb0c28a7a25bc3c
Publikováno v:
A&A 668, A13 (2022)
The latest Gaia Data Release 3 provides an opportunity to expand the census of Galactic open clusters harboring classical Cepheid variables, thereby bolstering the cosmic distance scale. A comprehensive analysis yielded a total of 50 classical Cephei
Externí odkaz:
http://arxiv.org/abs/2210.01521
Although a large number of Galactic open clusters (OCs) have been identified, the internal kinematic properties (e.g., rotation) of almost all the known OCs are still far from clear. With the high-precision astrometric data of Gaia EDR3, we have deve
Externí odkaz:
http://arxiv.org/abs/2210.01420