Zobrazeno 1 - 10
of 99
pro vyhledávání: '"LIU Jin-zhong"'
Autor:
Li, Chun, Fan, Zhou, Zhao, Gang, Wang, Wei, Zheng, Jie, Tan, Kefeng, Zhao, Jingkun, Huang, Yang, Yuan, Haibo, Xiao, Kai, Chen, Yuqin, Li, Haining, Liu, Yujuan, Song, Nan, Esamdin, Ali, Niu, Hu-Biao, Liu, Jin-Zhong, Feng, Guo-Jie
The Stellar Abundances and Galactic Evolution Survey (SAGES) is a multi-band survey that covers the northern sky area of ~12000 deg2. Nanshan One-meter Wide-field Telescope (NOWT) of Xinjiang Astronomical Observatory (XAO) carried out observations on
Externí odkaz:
http://arxiv.org/abs/2410.10218
Two Dynamically Discovered Compact Object Candidate Binary Systems from LAMOST Low-resolution Survey
We report two binary systems, LAMOST J035540+381550 (hereafter J035540) and LAMOST J035916+400732 (hereafter J035916), identified through the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) low-resolution survey (LRS). Each of thes
Externí odkaz:
http://arxiv.org/abs/2406.17340
The stellar spectra from LAMOST Medium Resolution Survey can be used to search for compact objects in binaries. The LAMOST DR10 catalog includes > 980, 000 targets with multiple medium resolution spectra. We select the targets with large or rapid rad
Externí odkaz:
http://arxiv.org/abs/2405.09825
Publikováno v:
口腔疾病防治, Vol 24, Iss 3, Pp 150-153 (2016)
Objective To investigate the expression of TKTL1 (transketolase-like protein 1) gene and its correlation with clinicopathological characteristics and prognosis of human tongue squamous cell carcinoma.Methods Immunohistochemistry was used to detect th
Externí odkaz:
https://doaj.org/article/955b07bec8c84a549be9607254c9e3de
Autor:
Shen, Dong-Xiang, Li, Gang, Abdusamatjan, Iskandar, Fu, Jian-Ning, Zhu, Chun-Hua, Yu, Jin-Long, Zhang, Yu, Lv, Guo-Liang, Zhai, Nan-Nan, Liu, Jin-Zhong
Magnetic hot stars refer to the stars, which effective temperatures approximately in the range from 7,000 to 50,000 K, and with large-scale globally organized magnetic fields. These magnetic fields exhibit strengths ranging from tens of Gauss to tens
Externí odkaz:
http://arxiv.org/abs/2308.15687
Autor:
Zhu, Zi-Pei, Lei, Wei-Hua, Malesani, Daniele B., Fu, Shao-Yu, Liu, Dong-Jie, Xu, Dong, D'Avanzo, Paolo, Fernández, José Feliciano Agüí, Fynbo, Johan P. U., Gao, Xing, Guelbenzu, Ana Nicuesa, Jiang, Shuai-Qing, Kann, David Alexander, Klose, Sylvio, Liu, Jin-Zhong, Liu, Xing, De Pasquale, Massimiliano, Postigo, Antonio de Ugarte, Stecklum, Bringfried, Th, Christina, Viuho, Joonas Kari Markku, Zhu, Yi-Nan, Li, Jing-Da, Gao, He, Lu, Tian-Hua, Xiao, Shuo, Zou, Yuan-Chuan, Xin, Li-Ping, Wei, Jian-Yan
High-redshift gamma-ray bursts (GRBs) provide a powerful tool to probe the early universe, but still for relatively few do we have good observations of the afterglow. We here report the optical and near-infrared observations of the afterglow of a rel
Externí odkaz:
http://arxiv.org/abs/2303.09982
Autor:
Zhu, Zi-Pei, Xu, Dong, Fynbo, Johan P. U., Fu, Shao-Yu, Liu, Xing, Jiang, Shuai-Qing, Xiao, Shuo, Xie, Wei, Zou, Yuan-Chuan, Gao, He, Hartmann, Dieter, Postigo, Antonio de Ugarte, Kann, David Alexander, Della Valle, Massimo, Jakobsson, Pall, Zafar, Tayabba, D'Elia, Valerio, Xin, Li-Ping, Wei, Jian-Yan, Gao, Xing, Liu, Jin-Zhong, Lu, Tian-Hua, Lei, Wei-Hua
Early optical observations of gamma-ray bursts can significantly contribute to the study of the central engine and physical processes therein. However, of the thousands observed so far, still only a few have data at optical wavelengths in the first m
Externí odkaz:
http://arxiv.org/abs/2302.09722
Autor:
Shen, Dong-Xiang, Liu, Jin-Zhong, Zhu, Chun-Hua, Lv, Guo-Liang, Zhang, Yu, Lv, Cheng-Long, Wang, Hao-Zhi, Li, Lei, Lu, Xi-Zhen, Yu, Jin-Long, Rustem, Abdurepqet
We first present the multicolor photometry results of the rapidly rotating magnetic star HD 345439 using the Nanshan One-meter Wide-field Telescope. From the photometric observations, we derive a rotational period of 0.7699\pm0.0014 day. The light cu
Externí odkaz:
http://arxiv.org/abs/2211.00271
Autor:
Xiao, Shuo, Zhang, Yan-Qiu, Zhu, Zi-Pei, Xiong, Shao-Lin, Gao, He, Xu, Dong, Zhang, Shuang-Nan, Peng, Wen-Xi, Li, Xiao-Bo, Zhang, Peng, Lu, Fang-Jun, Lin, Lin, Liu, Liang-Duan, Zhang, Zhen, Ge, Ming-Yu, Tuo, You-Li, Xue, Wang-Chen, Fu, Shao-Yu, Liu, Xing, Liu, Jin-Zhong, Li, An, Wang, Tian-Cong, Zheng, Chao, Wang, Yue, Jiang, Shuai-Qing, Li, Jin-Da, Liu, Jia-Cong, Cao, Zhou-Jian, Luo, Xi-Hong, Yang, Jiao-Jiao, Yi, Shu-Xu, Wang, Xi-Lu, Cai, Ce, Yi, Qi-Bin, Zhao, Yi, Xie, Sheng-Lun, Li, Cheng-Kui, Luo, Qi, Song, Li-Ming, Zhang, Shu, Qu, Jin-Lu, Liu, Cong-Zhan, Li, Xu-Fang, Xu, Yu-Peng, Li, Ti-Pei
Publikováno v:
ApJ 970 6 (2024)
The milestone discovery of GW 170817-GRB 170817A-AT 2017gfo has shown that gravitational wave (GW) could be produced during the merger of neutron star-neutron star/black hole and that in electromagnetic (EM) wave a gamma-ray burst (GRB) and a kilonov
Externí odkaz:
http://arxiv.org/abs/2205.02186
Autor:
Wang, Luqian, Li, Jiao, Wu, You, Gies, Douglas R., Liu, Jin Zhong, Liu, Chao, Guo, Yanjun, Chen, Xuefei, Han, Zhanwen
Be stars are B-type main-sequence stars that display broad Balmer emission lines in their spectra. Identification of Be population is essential to further examine the formation and evolutionary models. We report the detection of classical Be (CBe) st
Externí odkaz:
http://arxiv.org/abs/2203.15289