Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Qiao, E. L."'
Autor:
Zhao, S. J., Tao, L., Li, P. P., Soria, R., Feng, H., Zhang, Y. X., Ma, R. C., Zhang, W. D., Qiao, E. L., Yin, Q. Q., Zhang, S. N., Zhang, L., Bu, Q. C., Ma, X., Huang, Y., Ge, M. Y., Li, X. B., Zhao, Q. C., Peng, J. Q., Xiao, Y. X.
Publikováno v:
A&A 685, A42 (2024)
The black hole X-ray binary source 4U 1543--47 experienced a super-Eddington outburst in 2021, reaching a peak flux of up to $\sim1.96\times10^{-7}\rm erg\ \rm cm^{-2}\ \rm s^{-1}$ ($\sim 8.2$ Crab) in the 2--10\,keV band. Soon after the outburst beg
Externí odkaz:
http://arxiv.org/abs/2312.09632
Autor:
Li, P. P., Tao, L., Zhang, L., Bu, Q. C., Qu, J. L., Ji, L., Wang, P. J., Chen, Y. P., Zhang, S., Ma, R. C., Yang, Z. X., Ye, W. T., Zhao, S. J., Zhao, Q. C., Huang, Y., Ma, X., Qiao, E. L., Jia, S. M., Zhang, S. N.
MAXI J181-195 is a newly discovered accreting millisecond X-ray pulsar that went outburst in June 2022. Through timing analysis with NICER and NuSTAR observations, we find a transient modulation at ~2.5 Hz during the decay period of MAXI J1816-195. T
Externí odkaz:
http://arxiv.org/abs/2307.13955
Autor:
Ma, R. C., Soria, R., Tao, L., Zhang, W., Qu, J. L., Zhang, S. N., Zhang, L., Qiao, E. L., Zhao, S. J., Ge, M. Y., Li, X. B., Huang, Y., Song, L. M., Zhang, S., Bu, Q. C., Wang, Y. N., Ma, X., Jia, S. M.
We studied the transient Galactic black hole candidate MAXI J0637-430 with data from Insight-HXMT, Swift and XMM-Newton. The broad-band X-ray observations from Insight-HXMT help us constrain the power-law component. MAXI J0637-430 is located at unusu
Externí odkaz:
http://arxiv.org/abs/2206.03409
Autor:
Zhao, S. J., Tao, L., Li, P. P., Soria, R., Feng, H., Zhang, Y. X., Ma, R. C., Zhang, W. D., Qiao, E. L., Yin, Q. Q., Zhang, S. N., Zhang, L., Bu, Q. C., Ma, X., Huang, Y., Ge, M. Y., Li, X. B., Chen, L., Zhao, Q. C., Peng, J. Q.
Publikováno v:
Astronomy & Astrophysics / Astronomie et Astrophysique; 5/3/2024, Vol. 685, p1-14, 14p
In this paper, we consider the effect of Landau levels on the decay of superhigh magnetic fields of magnetars. Applying ${}^3P_2$ anisotropic neutron superfluid theory yield a second-order differential equation for a superhigh magnetic field $B$ and
Externí odkaz:
http://arxiv.org/abs/1312.2728
We investigate the accretion process in high-luminosity AGNs (HLAGNs) in the scenario of the disk evaporation model. Based on this model, the thin disk can extend down to the innermost stable circular orbit (ISCO) at accretion rates higher than $0.02
Externí odkaz:
http://arxiv.org/abs/1205.6958
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Autor:
Li, P P, Tao, L, Zhang, L, Bu, Q C, Qu, J L, Ji, L, Wang, P J, Chen, Y P, Zhang, S, Ma, R C, Yang, Z X, Ye, W T, Zhao, S J, Zhao, Q C, Huang, Y, Ma, X, Qiao, E L, Jia, S M, Zhang, S N
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 10/15/2023, Vol. 525 Issue 1, p595-606, 12p
Autor:
Zhao, Q C, Yin, H X, Tao, L, Yang, Z X, Qu, J L, Zhang, L, Zhang, S, Qiao, E L, Bu, Q C, Zhao, S J, Li, P P, Huang, Y M, Ma, R C, Tang, R J, Jin, P, Yu, W, Liu, H X, Huang, Y, Ma, X, Xiao, J Y
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Sep2023, Vol. 524 Issue 3, p3215-3230, 16p