中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
机构
采集方式
内容类型
发表日期
学科主题
筛选

浏览/检索结果: 共52条,第1-10条 帮助

条数/页: 排序方式:
Evolution of orphan and atypical histidine kinases and response regulators for microbial signaling diversity 期刊论文  OAI收割
INTERNATIONAL JOURNAL OF BIOLOGICAL MACROMOLECULES, 2024, 卷号: 275, 页码: 14
作者:  
Xu, Gangming;  Yang, Suiqun
  |  收藏  |  浏览/下载:4/0  |  提交时间:2024/09/02
The TorRS two component system regulates expression of TMAO reductase in response to high hydrostatic pressure in Vibrio fluvialis 期刊论文  OAI收割
FRONTIERS IN MICROBIOLOGY, 2023, 卷号: 14, 页码: 10
作者:  
  |  收藏  |  浏览/下载:26/0  |  提交时间:2023/12/25
A Star-Identification Algorithm Based on Global Multi-Triangle Voting 期刊论文  OAI收割
APPLIED SCIENCES-BASEL, 2022, 卷号: 12, 期号: 19
作者:  
  |  收藏  |  浏览/下载:51/0  |  提交时间:2022/10/25
A novel copper-sensing two-component system for inducing Dsb gene expression in bacteria 期刊论文  OAI收割
SCIENCE BULLETIN, 2022, 卷号: 67, 期号: 2, 页码: 198-212
作者:  
Yu, Liang;  Cao, Qiao
  |  收藏  |  浏览/下载:51/0  |  提交时间:2022/06/15
FixJ family regulator AcfR of Azorhizobium caulinodans is involved in symbiosis with the host plant 期刊论文  OAI收割
BMC MICROBIOLOGY, 2021, 卷号: 21, 期号: 1, 页码: 9
作者:  
Liu, Wei;  Bai, Xue;  Li, Yan;  Zhang, Haikun;  Hu, Xiaoke
  |  收藏  |  浏览/下载:48/0  |  提交时间:2021/06/07
Genome-Wide Mapping Reveals Complex Regulatory Activities of BfmR in Pseudomonas aeruginosa 期刊论文  OAI收割
MICROORGANISMS, 2021, 卷号: 9, 期号: 3, 页码: 22
作者:  
Fan, Ke;  Cao, Qiao;  Lan, Lefu
  |  收藏  |  浏览/下载:29/0  |  提交时间:2021/05/24
Glucose-Binding of Periplasmic Protein GltB Activates GtrS-GltR Two-Component System in Pseudomonas aeruginosa 期刊论文  OAI收割
MICROORGANISMS, 2021, 卷号: 9, 期号: 2, 页码: 28
作者:  
Xu, Chenchen;  Cao, Qiao;  Lan, Lefu
  |  收藏  |  浏览/下载:30/0  |  提交时间:2021/05/24
Evaluating the Impacts of Universal Two-Child Policy on Beijing's Population 期刊论文  OAI收割
JOURNAL OF SYSTEMS SCIENCE & COMPLEXITY, 2020, 页码: 18
作者:  
Liu, Qing;  Liu, Xiuli
  |  收藏  |  浏览/下载:29/0  |  提交时间:2020/06/30
Identification of potential drug-targets by combining evolutionary information extracted from frequency profiles and molecular topological structures 期刊论文  OAI收割
CHEMICAL BIOLOGY & DRUG DESIGN, 2020, 卷号: 96, 期号: 2, 页码: 758-767
作者:  
Wang, L (Wang, Lei)[ 1,2 ];  You, ZH (You, Zhu-Hong)[ 2 ];  Li, LP (Li, Li-Ping)[ 2 ];  Yan, X (Yan, Xin)[ 3 ];  Zhang, W (Zhang, Wei)[ 1 ]
  |  收藏  |  浏览/下载:30/0  |  提交时间:2020/11/04
The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition 期刊论文  OAI收割
Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 494, 页码: 1865-1870
作者:  
HXMT
  |  收藏  |  浏览/下载:64/0  |  提交时间:2022/02/08
stars: magnetic field  stars: neutron  pulsars: general  Astrophysics  - High Energy Astrophysical Phenomena  Abstract: In 2011 December, PSR B054-69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by $\sim 36{{\ \rm per\ cent}}$. About 1000 d after the SRT, the X-ray luminosity of the associated pulsar wind nebula (PWN) was found to brighten by $32\pm 8{{\ \rm per\ cent}}$. After the SRT, the braking index n of PSR B0540-69 changes from n = 2.12 to 0.03 and then keeps this value for about five years before rising to n = 0.9 in the following years. We find that most of the current models have difficulties in explaining the measured braking index. One exceptive model of the braking index evolution is the increasing dipole magnetic field of PSR B0540-69. We suggest that the field increase may result from some instabilities within the pulsar core that enhance the poloidal component at the price of toroidal component of the magnetic field. The increasing dipole magnetic field will result in the X-ray brightening of the PWN. We fit the PWN X-ray light curve by two models: one assumes a constant magnetic field within the PWN during the brightening and the other assumes an enhanced magnetic field proportional to the energy density of the PWN. It appears that the two models fit the data well, though the later model seems to fit the data a bit better. This provides marginal observational evidence that magnetic field in the PWN is generated by the termination shock. Future high-quality and high-cadence data are required to draw a solid conclusion.