Zobrazeno 1 - 10
of 90
pro vyhledávání: '"Y. L. Tuo"'
Autor:
Y. X. Xiao, Y. J. Xu, M. Y. Ge, F. J. Lu, S. N. Zhang, S. Zhang, L. Tao, J. L. Qu, P. J. Wang, L. D. Kong, Y. L. Tuo, Y. You, S. J. Zhao, J. Q. Peng, Y. F. Du, Y. H. Zhang, W. T. Ye
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 1, p 18 (2024)
We report the phase-resolved spectral results of the first Galactic pulsating ultraluminous X-ray source (PULX) Swift J0243.6+6124, modeling its 2017–2018 outburst peak using data collected by the Hard X-ray Modulation Telescope (Insight-HXMT). The
Externí odkaz:
https://doaj.org/article/207301a8b77c471a8c3a45ee824a2e7a
Autor:
G. C. Xiao, R. Staubert, L. Ji, M. Y. Ge, Q. Z. Liu, J. L. Qu, S. Zhang, S. N. Zhang, J. Z. Yan, J. Li, Q. C. Bu, Y. L. Tuo, H. X. Liu, Z. X. Yang
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 1, p 57 (2023)
Recent observations of Her X-1 with NuSTAR (as well as with INTEGRAL, Swift, and Astrosat) have provided evidence that the nearly 20 yr-long decay of the cyclotron line energy since ∼1994 has ended and that a stable value has replaced the decay. Us
Externí odkaz:
https://doaj.org/article/db49aa539fab42228e5b744c8bb8dc32
Autor:
M. Y. Ge, C. Z. Liu, S. N. Zhang, F. J. Lu, Z. Zhang, Z. Chang, Y. L. Tuo, X. B. Li, C. K. Li, S. L. Xiong, C. Cai, X. F. Li, R. Zhang, Z. G. Dai, J. L. Qu, L. M. Song, S. Zhang, L. J. Wang
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 1, p 67 (2023)
A double-peak X-ray burst from the Galactic magnetar SGR J1935+2154 was discovered to be associated with the two radio pulses of FRB 200428 separated by 28.97 ± 0.02 ms. Precise measurements of the timing and spectral properties of the X-ray bursts
Externí odkaz:
https://doaj.org/article/02de0983a4fb4f1badf4990614982acb
Autor:
G. Q. Ding, J. L. Qu, L. M. Song, Y. Huang, S. Zhang, Q. C. Bu, M. Y. Ge, X. B. Li, L. Tao, X. Ma, Y. P. Chen, L. Zhang, W. M. Yan, Y. L. Tuo, Y. C. Fu, S. H. Xiao, Z. X. Yang, H. X. Liu
Publikováno v:
The Astrophysical Journal, Vol 950, Iss 1, p 69 (2023)
Using the observations of the high-energy detector of the Hard X-ray Modulation Telescope (Insight-HXMT) for Scorpius X-1 from 2017 to 2020, we search for hard X-ray tails in the X-ray spectra in ∼30–200 keV. The hard X-ray tails are found throug
Externí odkaz:
https://doaj.org/article/2585e15983ec4ffe93f1a27655c16752
Akademický článek
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Autor:
P J Wang, L D Kong, Y P Chen, S Zhang, S N Zhang, R Soria, L Ji, J L Qu, Y Huang, L Tao, M Y Ge, F J Lu, L Chen, T P Li, Y P Xu, X L Cao, Y Chen, C Z Liu, Q C Bu, C Cai, Z Chang, T X Chen, Y B Chen, W W Cui, Y Y Du, G H Gao, H Gao, Y D Gu, J Guan, C C Guo, D W Han, J Huo, S M Jia, W C Jiang, J Jin, B Li, C K Li, G Li, W Li, X Li, X B Li, X F Li, Z W Li, X H Liang, J Y Liao, B S Liu, H X Liu, H W Liu, X J Liu, X F Lu, Q Luo, T Luo, R C Ma, X Ma, B Meng, Y Nang, J Y Nie, G Ou, X Q Ren, N Sai, L M Song, X Y Song, L Sun, Y Tan, Y L Tuo, C Wang, L J Wang, W S Wang, Y S Wang, X Y Wen, B Y Wu, B B Wu, M Wu, G C Xiao, S Xiao, S L Xiong, R J Yang, S Yang, Yan Ji Yang, Yi Jung Yang, Q B Yi, Q Q Yin, Y You, F Zhang, H M Zhang, J Zhang, P Zhang, W C Zhang, W Zhang, Y F Zhang, Y H Zhang, H S Zhao, X F Zhao, S J Zheng, Y G Zheng, D K Zhou
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:4541-4555
We studied the 2018 outburst of the black hole transient H 1743 − 322 with a series of Insight-HXMT, NICER, and NuSTAR observations, covering the 1–120 keV band. With our broad-band X-ray spectral modelling, we confirm that the source remained in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8274eef826abbaa57ae568ce1f6c2f65
https://doi.org/10.1093/mnras/stac773
https://doi.org/10.1093/mnras/stac773
Autor:
S Xiao, Y Q Liu, W X Peng, Z H An, S L Xiong, Y L Tuo, K Gong, P Zhang, K Zhang, S J Zheng, C Y Li, M Gao, D Y Guo, X Q Li, X H Liang, X J Liu, R Qiao, X L Sun, J Z Wang, X Y Wen, Y B Xu, S Yang, D L Zhang, Fan Zhang, Fei Zhang, X Y Zhao, J L Qi, X B Han, Z D Li, J Huang, L M Song, C Cai, Q B Yi, Y Zhao, X Y Song, Y Huang, M Y Ge, X Ma, X B Li, B Li, P Wang, J Wang, Y Q Zhang, Z Zhang, X L Zhang, H Y Zhao, Z W Guo, C Chen, S L Xie, S N Zhang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 511:964-971
High time resolution and accuracy are of critical importance in the studies of timing analysis and time delay localization of gamma-ray bursts (GRBs), soft gamma-ray repeaters (SGRs) and pulsars. The Gravitational wave high-energy Electromagnetic Cou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1052852382a306620d972dda03f4f934
https://doi.org/10.1093/mnras/stac085
https://doi.org/10.1093/mnras/stac085
Autor:
Yu-Cong Fu, L M Song, G Q Ding, M Y Ge, Y L Tuo, S Zhang, S N Zhang, X Hou, J L Qu, J Zhang, L Zhang, Q C Bu, Y Huang, X Ma, X Zhou, W M Yan, Z X Yang, X F Lu, T M Li, Y C Xu, P J Wang, S H Xiao, H X Liu, X Q Ren, Y F Du, Q X Zhao, Y X Xiao
We report the evolution of the X-ray pulsations of EXO 2030+375 during its 2021 outburst using the observations from Insight-HXMT. Based on the accretion torque model, we study the correlation between the spin frequency derivatives and the luminosity
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c22758e6fd5cd8155c06761474d30414
http://arxiv.org/abs/2302.02167
http://arxiv.org/abs/2302.02167
Autor:
X. Hou, Y. You, L. Ji, R. Soria, S. N. Zhang, M. Y. Ge, L. Tao, S. Zhang, H. Feng, M. Zhou, Y. L. Tuo, L. M. Song, J. C. Wang
Pulsating ultraluminous X-ray sources (PULXs) are accreting pulsars with apparent X-ray luminosity exceeding $10^{39}\, \rm erg\ s^{-1}$. We perform Monte-Carlo simulations to investigate whether high collimation effect (or strong beaming effect) is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5474102215cdfc9c6ce0216da372786e
http://arxiv.org/abs/2211.08021
http://arxiv.org/abs/2211.08021
Autor:
X. Q. Ren, Yanan Wang, S. N. Zhang, R. Soria, L. Tao, L. Ji, Y. J. Yang, J. L. Qu, S. Zhang, L. M. Song, M. Y. Ge, Y. Huang, X. B. Li, J. Y. Liao, H. X. Liu, R. C. Ma, Y. L. Tuo, P. J. Wang, W. Zhang, D. K. Zhou
We study the spectral evolution of the black hole candidate EXO 1846$-$031 during its 2019 outburst, in the 1--150 keV band,with the {\it {Hard X-ray Modulation Telescope}}. The continuum spectrum is well modelled with an absorbed disk-blackbody plus
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dff585011eab3b279dcc5781a75592ad
https://eprints.soton.ac.uk/474867/
https://eprints.soton.ac.uk/474867/