Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Wei-Jian LU"'
Autor:
Ding-Pei Long, Ai-Chun Zhao, Xue-Jiao Chen, Yang Zhang, Wei-Jian Lu, Qing Guo, Alfred M Handler, Zhong-Huai Xiang
Publikováno v:
PLoS ONE, Vol 7, Iss 6, p e40150 (2012)
A comprehensive understanding of gene function and the production of site-specific genetically modified mutants are two major goals of genetic engineering in the post-genomic era. Although site-specific recombination systems have been powerful tools
Externí odkaz:
https://doaj.org/article/3a908ede7c564abe8f2810c243c55b84
Autor:
Ying-Ru Lin, Wei-Jian Lu
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 497:1457-1462
Rodríguez Hidalgo et al. (2013, ApJ, 775, 14) have reported the transition of a C iv mini-broad absorption line (mini-BAL) into a BAL in quasar SDSS J115122.14+020426.3 (hereafter J1151+0204). Based on the two-epoch spectra obtained from the Sloan D
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8fd7fd4bfd961542301305bc12e23bf8
https://doi.org/10.1093/mnras/staa2037
https://doi.org/10.1093/mnras/staa2037
Autor:
Wei, Jian‐lu1,2 (AUTHOR), Zhu, Yan‐bin2,3 (AUTHOR), Zhao, Da‐wang1 (AUTHOR), Chen, Wei2,3 (AUTHOR), Wang, Juan2,3 (AUTHOR), Wang, Hong4 (AUTHOR), Lv, Jia‐li5 (AUTHOR), Zhang, Tao5 (AUTHOR), Cheng, Lei1 (AUTHOR), Zhang, Ying‐ze2,3 (AUTHOR) dr_yzzhang@126.com
Publikováno v:
Orthopaedic Surgery. Dec2019, Vol. 11 Issue 6, p1072-1081. 10p.
Autor:
Ying-Ru Lin, Wei-Jian Lu
We report, for the first time, a synchronized velocity shift of Mg II and Al III broad absorption lines (BALs) in quasar SDSS J134444.33+315007.6 (hereafter J1344+3150). We found this quasar from a sample of 134 Mg II BAL quasars with multi-epoch obs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3bd0b42b57eaf734bc397f061fb6a5ce
Autor:
Yi-Ping Qin, Wei-Jian Lu
Publikováno v:
Research in Astronomy and Astrophysics. 21:261
As the advent of precision cosmology, the Hubble constant ($H_0$) inferred from the Lambda Cold Dark Matter fit to the Cosmic Microwave Background data is increasingly in tension with the measurements from the local distance ladder. To approach its r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d1b9f498aba1aa6405086479864107c
https://doi.org/10.1088/1674-4527/21/10/261
https://doi.org/10.1088/1674-4527/21/10/261
Autor:
Cai-Juan Pan, Hong-Yan Huang, Zhi-Kao Yao, Wei-Jing Nong, Wei-Jian Lu, Yi-Ping Qin, Yu-Tao Zhou, Ying-Ru Lin, Qing-Lin Han, Wei-Rong Huang, Mei-Mei Lu, Min Yao
Correlations between the variations of quasar absorption lines and the ionizing continuum have been confirmed recently in systematic studies. However, no convincing individual case is reported. We present a statistical analysis of the variable C iv b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eda46932858b7ec626d67fa03782de1c
http://arxiv.org/abs/1905.02407
http://arxiv.org/abs/1905.02407
Autor:
Wei-Jian Lu, Ying-Ru Lin
We discover the significant (significance level of >99%) correlations between the fractional variation of the ionizing continuum and that of the C IV and/or Si IV BALs in each of 21 BAL quasars that have at least five-epoch observations from the Sloa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ac147cbc5007c5dfc282f1e7f7a4e221
Autor:
Ying-Ru Lin, Wei-Jian Lu
We report the kinematic shift of the C IV broad absorption line (BAL) in quasar SDSS J120819.29+035559.4 (hereafter J1208+0355). This quasar shows two BAL systems, including a blue component of system A at $\sim$-23500$\,\rm km\,s^{-1}$ that shows a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::217d45c7fd44abca26157fc8bfa5e4c0
Narrow Absorption Lines Complex. III. Gradual Transition from Type S to Type N Broad Absorption Line
Autor:
Wei-Jian Lu, Ying-Ru Lin
We study the relationship between the broad absorption lines (BALs) that can be decomposed into multiple narrow absorption lines and those that cannot (hereafter Type N and Type S BAL, respectively), based on the analysis of three BAL systems (system
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f44205ad049914b83bf960bc6674288
Autor:
Ying-Ru Lin, Wei-Jian Lu
Publikováno v:
The Astrophysical Journal. 899:155
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d0b4d37b792c4fb16d0c9d82670a0455
https://doi.org/10.3847/1538-4357/aba9db
https://doi.org/10.3847/1538-4357/aba9db