Zobrazeno 1 - 10
of 6 440
pro vyhledávání: '"Bi S"'
Publikováno v:
The Application of Clinical Genetics, Vol Volume 17, Pp 63-69 (2024)
Ying Wang, Shaohua Bi, Xiaoqing Shi, Liying Dai Division of Neonatology, Anhui Provincial Children’s Hospital, Hefei, Anhui, 230051, People’s Republic of ChinaCorrespondence: Liying Dai, Division of Neonatology, Anhui Province Children’s Hospit
Externí odkaz:
https://doaj.org/article/1154d6e5107c4877a808868b6f2d0901
Publikováno v:
Cancer Management and Research, Vol Volume 11, Pp 10269-10274 (2019)
Rongxin Chen,1,* Huijing Ye,1,* Shu Liu,2,* Yueyan Lin,1 Wei Xiao,1 Shaowei Bi,1 Guo Chen,1 Te Zhang,1 Jingqiao Chen,1 Huasheng Yang1 1State Key Laboratory of Ophthalmology, Zhongshan Ophthalmic Center, Sun Yat-sen University, Guangzhou 510060, Peopl
Externí odkaz:
https://doaj.org/article/e2a000b47d3a4d30ae32fb054b606c00
Publikováno v:
Patient Preference and Adherence, Vol 2014, Iss default, Pp 1449-1455 (2014)
Shuping Zhao,1 Jihong Deng,2 Yan Wang,3 Shiliang Bi,4 Xiaoye Wang,5 Wen Qin,6 Zirong Huang,7 Li Li,8 Xin Mi,9 Liping Han,10 Qing Chang,11 Jian Li12 1The Affiliated Hospital of the Medical College Qingdao University, Qingdao, 2Kunming Maternal and Chi
Externí odkaz:
https://doaj.org/article/ee489b1e4dcf47c4ae3a943f80ca83da
Publikováno v:
Zeitschrift für Kristallographie - New Crystal Structures, Vol 219, Iss 1-4, Pp 447-448 (2004)
Externí odkaz:
https://doaj.org/article/c0a5853ed985475daf87497b91cd9e3f
Publikováno v:
In Materials Today Nano August 2023 23
Autor:
Bi, S., Jin, W., Han, X., Metts, J., Ostrosky, A.D., Lehotsky, J., He, Z., Jiang, C., Asare-Yeboah, K.
Publikováno v:
In Materials Today Sustainability March 2023 21
Publikováno v:
In Journal for Nature Conservation December 2022 70
Publikováno v:
In Materials Today Sustainability November 2022 19
Publikováno v:
MNRAS,2015,680,90
We intent to use stellar models with and without alpha-enhancement, as well as asteroseismic analysis, to study two alpha-enhanced stars, KIC 7976303 and KIC 8694723. For the alpha-enhanced models, we adopt [alpha/Fe] = 0.2, and 0.4. For the evolved
Externí odkaz:
http://arxiv.org/abs/1612.01280
Autor:
Ge, Z. S., Bi, S. L., Chen, Y. Q., Li, T. D., Zhao, J. K., Liu, K., W., Fergusion J., Wu, Y. Q.
Oxygen and carbon are important elements in stellar populations. Their behavior refers to the formation history of the stellar populations. C and O abundances would also obviously influence stellar opacities and the overall metal abundance $Z$. With
Externí odkaz:
http://arxiv.org/abs/1612.01622