Zobrazeno 1 - 10
of 149
pro vyhledávání: '"Zhao, XueShan"'
Autor:
Wang, Shiyu a, b, 1, Zhao, Xueshan a, 1, Zhang, Linna b, Dai, Kang d, Zhang, Zhenyu c, ⁎, Wang, Haibo b, Gu, Jun a, ⁎
Publikováno v:
In Chemical Engineering Journal 15 January 2025 504
Autor:
Bi, Siwei, He, Changyuan, Zhou, Yannan, Liu, Ruiqi, Chen, Chong, Zhao, Xueshan, Zhang, Li, Cen, Ying, Gu, Jun, Yan, Bin
Publikováno v:
In Biomaterials March 2025 314
Autor:
Jia, Nan, Zhao, Xueshan, Gou, Lijun, Garcia, Javier A., Liao, Zhenxuan, Feng, Ye, Li, Yufeng, Wang, Yuan, Li, Huixian, Wu, Jianfeng
The black hole candidate MAXI J1348-630 was discovered on January 26th, 2019, with the Gas Slit Camera (GSC) on-board \textit{MAXI}. We report a detailed spectral analysis of this source by using the archived data of \textit{NuSTAR}. A total of 9 obs
Externí odkaz:
http://arxiv.org/abs/2201.01207
MAXI J1803-298, a newly-discovered Galactic transient and black hole candidate, was first detected by \emph{MAXI}/GSC on May 1st, 2021. In this paper, we present a detailed spectral analysis of MAXI J1803-298. Utilizing the X-ray reflection fitting m
Externí odkaz:
http://arxiv.org/abs/2112.02794
Autor:
Feng, Ye, Zhao, Xueshan, Gou, Lijun, Wu, Jianfeng, Steiner, James F., Li, Yufeng, Liao, Zhenxuan, Jia, Nan, Wang, Yuan
As a transient X-ray binary, MAXI J1659-152 contains a black hole candidate as its compact star. MAXI J1659-152 was discovered on 2010 September 25 during its only known outburst. Previously-published studies of this outburst indicate that MAXI J1659
Externí odkaz:
http://arxiv.org/abs/2112.03479
Autor:
Feng, Ye, Zhao, Xueshan, Gou, Lijun, Li, Yufeng, Steiner, James F., García, Javier A., Wang, Yuan, Jia, Nan, Liao, Zhenxuan, Li, Huixian
AT2019wey is a new galactic X-ray binary that was first discovered as an optical transient by the Australia Telescope Large Area Survey (ATLAS) on December 7, 2019. AT2019wey consists of a black hole candidate as well as a low-mass companion star ($M
Externí odkaz:
http://arxiv.org/abs/2109.07357
Autor:
He, Changyuan, Bi, Siwei, Zhang, Rongya, Chen, Chong, Liu, Ruiqi, Zhao, Xueshan, Gu, Jun, Yan, Bin
Publikováno v:
In Journal of Controlled Release June 2024 370:543-555
Autor:
Zhao, Xueshan, Gou, Lijun, Dong, Yanting, Zheng, Xueying, Steiner, James F., Miller-Jones, James C. A., Bahramian, Arash, Orosz, Jerome A., Feng, Ye
Cygnus X-1 is a well-studied persistent black hole X-ray binary. Recently, the three parameters needed to estimate the black hole spin of this system, namely the black hole mass $M$, the orbital inclination $i$ and the source distance $D$, have been
Externí odkaz:
http://arxiv.org/abs/2102.09093
Autor:
Miller-Jones, James C. A., Bahramian, Arash, Orosz, Jerome A., Mandel, Ilya, Gou, Lijun, Maccarone, Thomas J., Neijssel, Coenraad J., Zhao, Xueshan, Ziółkowski, Janusz, Reid, Mark J., Uttley, Phil, Zheng, Xueying, Byun, Do-Young, Dodson, Richard, Grinberg, Victoria, Jung, Taehyun, Kim, Jeong-Sook, Marcote, Benito, Markoff, Sera, Rioja, María J., Rushton, Anthony P., Russell, David M., Sivakoff, Gregory R., Tetarenko, Alexandra J., Tudose, Valeriu, Wilms, Joern
The evolution of massive stars is influenced by the mass lost to stellar winds over their lifetimes. These winds limit the masses of the stellar remnants (such as black holes) that the stars ultimately produce. We use radio astrometry to refine the d
Externí odkaz:
http://arxiv.org/abs/2102.09091
Autor:
Zhao, Xueshan, Gou, Lijun, Dong, Yanting, Tuo, Youli, Liao, Zhenxuan, Li, Yufeng, Jia, Nan, Feng, Ye, Steiner, James F.
MAXI J1820+070 is a newly-discovered black hole X-ray binary, whose dynamical parameters, namely the black hole mass, the inclination angle and the source distance, have been estimated recently. \emph{Insight}-HXMT have observed its entire outburst f
Externí odkaz:
http://arxiv.org/abs/2012.05544