Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Bi-Xuan Zhao"'
Autor:
Dong-Wei Bao, Michael S. Brotherton, Pu Du, Jacob N. McLane, T. E. Zastrocky, Kianna A. Olson, Feng-Na Fang, Shuo Zhai, Zheng-Peng Huang, Kai Wang, Bi-Xuan Zhao, Sha-Sha Li, Sen Yang, Yong-Jie Chen, Jun-Rong Liu, Zhu-Heng Yao, Yue-Chang Peng, Wei-Jian Guo, Yu-Yang Songsheng, Yan-Rong Li, Bo-Wei Jiang, David H. Kasper, William T. Chick, My L. Nguyen, Jaya Maithil, H. A. Kobulnicky, D. A. Dale, Derek Hand, C. Adelman, Z. Carter, A. M. Murphree, M. Oeur, S. Schonsberg, T. Roth, Hartmut Winkler, Paola Marziani, Mauro D’Onofrio, Chen Hu, Ming Xiao, Suijian Xue, Bożena Czerny, Jesús Aceituno, Luis C. Ho, Jin-Ming Bai, Jian-Min Wang
Full list of authors: Bao, Dong-Wei; Brotherton, Michael S.; Du, Pu; McLane, Jacob N.; Zastrocky, T. E.; Olson, Kianna A.; Fang, Feng-Na; Zhai, Shuo; Huang, Zheng-Peng; Wang, Kai; Zhao, Bi-Xuan; Li, Sha-Sha; Yang, Sen; Chen, Yong-Jie; Liu, Jun-Rong;
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c78424c2a40266f88c5cc1936194ce3
http://hdl.handle.net/10261/285262
http://hdl.handle.net/10261/285262
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:1519-1534
Using a compiled sample of 34 broad-line active galactic nuclei (AGNs) with measured H$\beta$ time lags from the reverberation mapping (RM) method and measured bulge stellar velocity dispersions $\sigma_*$, we calculate the virial factor $f$ by assum
Autor:
Chan Wang, Bi-Xuan Zhao, Bing-Qian Zhu, Yu-Qin Chen, Xue-Guang Zhang, Xue Ge, Li-Ming Yu, Wei-Hao Bian
Using different kinds of velocity tracers derived from the broad H$\beta$ profile (in the mean or rms spectrum) and the corresponding virial factors $f$, the central supermassive black hole (SMBH) masses ($M_{\rm BH}$) are calculated for a compiled s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e380db2e2adeced74464d2b875dc9a5
http://arxiv.org/abs/2008.06623
http://arxiv.org/abs/2008.06623
Publikováno v:
Astrophysics and Space Science. 365
The variability of the UV and optical Fe ii emission is investigated for a QSO, SDSS J142052.43+525622.4 ($z = 0.676$), with 50 spectroscopic observations covering 1047 d in the observed frame. This QSO is selected from the Sloan Digital Sky Survey-R
Publikováno v:
Research in Astronomy and Astrophysics. 22:015012
The 21 CentiMeter Array (21CMA) is a radio interferometer in western China. The key science objective of 21CMA is statistically measuring the redshifted H i 21 cm signal of the Epoch of Reionization (EoR). In order to achieve this, a catalog of radio
For a compiled sample of 120 reverberation-mapped AGNs, the bivariate correlations of the broad-line regions (BLRs) size ($R_{\rm BLR}$) with the continuum luminosity at 5100 \AA\ ($L_{5100}$) and the dimensionless accretion rates ($\dot{\mathscr{M}}
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fcd85421f74c425db4a541961f1d79c5
http://arxiv.org/abs/1911.10802
http://arxiv.org/abs/1911.10802
Incorporating the radiation reaction force into two-fluid plasma in curved space, we get a set of one-fluid general relativistic magnetohydrodynamics (GRMHD) equations with the Landau-Lifshitz radiation reaction force. We analyze the importance of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a60bba9b163492efbf5eb59eaea08468
http://arxiv.org/abs/1906.08955
http://arxiv.org/abs/1906.08955
Using a sample of 208 broad-line active galactic nuclei (AGNs) from Swift/BAT AGN Spectroscopic Survey in ultra-hard X-ray band ($14-195$ keV), the hot corona properties are investigated, i.e. the fraction of gravitational energy dissipated in the ho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b2cce466d348a694e80bed4e54e2b20
By taking into account the radiation reaction force, we derive a set of one-fluid relativistic magnetohydrody-namics (RMHD) equations with the Landau-Lifshitz radiation reaction force based on a relativistic two-fluid plasma. These equations could be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::56880cff8627e802ba806215e459c67c
http://arxiv.org/abs/1811.03989
http://arxiv.org/abs/1811.03989
Publikováno v:
The Astronomical Journal. 157:148
For the sample from Ge et al. of 87 low-$z$ Palomar--Green (PG) quasi-stellar objects (QSOs) and 130 high-$z$ QSOs ($0
Comment: 18 pages, 8 figures, Accepted for publication in AJ
Comment: 18 pages, 8 figures, Accepted for publication in AJ