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supported by the National Key Research and Development Programs of China(2022YFF0711404,2021YFA0718500,2022SKA0130102,2022SKA0130100);supported by the Strategic Priority Program on Space Science,led by CAS(XDA15310000,XDA15052100);supported by the Strategic Priority Research Program on Space Science,led by CAS(XDA15360000,XDA15360102,XDA15360300,XDA15052700);support from the National Natural Science Foundation of China(11833003,U2038105,12121003,12173055,11922301,12041306,12103089,12203071,12103065,12273042,12173038,12173056,12333007,12027803 and 13001106);the China Manned Space Project under research grant CMS-CSST-2021-B11,the Natural Science Foundation of Jiangsu Province(BK20211000);the International Partnership Program of the Chinese Academy of Sciences for Grand Challenges(114332KYSB20210018);the Major Science and Technology Project of Qinghai Province(2019-ZJ-A10);the Youth Innovation Promotion Association of the Chinese Academy of Sciences,the Postgraduate Research&Practice Innovation Program of Jiangsu Province(KYCX23_0117);the Program for Innovative Talents,Entrepreneur in Jiangsu,and the International Partnership Program of the Chinese Academy of Sciences(113111KYSB20190020).
The central engine that powers gamma-ray bursts(GRBs),the most powerful explosions in the universe,is still not identified.Besides hyper-accreting black holes,rapidly spinning and highly magnetized neutron stars,known...
Supported by the National Natural Science Fund of China(12005184,12175192,12275034,12347101);the Fundamental Research Funds for the Central Universities of China(2024CDJXY-022)。
The time series of energy and waiting time in magnetar bursts carry important information about the source activity.In this study,we investigate the memory and dynamical stability of magnetar bursts from four soft gam...
How gamma-ray bursts(GRBs),the most powerful and spectacular explosions known in the universe since the Big Bang,fuel their high-energy radiations?What kind of physical reactions can trigger and sustain such violent,e...
supported by the Guangxi Science Foundation(grant No.2023GXNSFDA026007);the Program of Bagui Scholars Program(LHJ)。
Theoretically,a supra-massive neutron star or magnetar may be formed after the merger of binary neutron stars.GRB210323A is a short-duration gamma-ray burst(GRB)with a duration of lasting~1 s.The light curve of the pr...
funded by the National Natural Science Foundation of China(Nos.12373042,U1938201,12273005 and 12133003);the Programme of Bagui Scholars Programme(WXG);support of the China Space Station Telescope(CSST)。
After launching a jet,outflows of magnetar were used to account for the achromatic plateau of afterglow and the early X-ray flux plateau known as“internal plateau”.The lack of detecting magnetic dipole emission toge...
Supported by the Changsha Municipal Natural Science Foundation(kq2007004);the Science Research Key Project of Education Department of Hunan Province(21A0186);the Construct Program of the Key Discipline in Hunan Province,China。
We explore the properties of 4110 nuclides from Z=5 to Z=82 with the Sky3D code and the composition of the outer crust in magnetars under extreme magnetic fields.The effects of the variation in nuclear masses due to m...
supported by International Partnership Program of Chinese Academy of Sciences(grant No.113111KYSB20190020);by the National Key R&D Program of China(2021YFA0718500)from the Minister of Science and Technology of China(MOST);supports from the National Natural Science Foundation of China under Grants U1938109,12333007,12173103,U2038101,U1938103,12333007,12303045,U1938201 and 11733009。
In October 2022,the magnetar SGR J1935+2154 entered the active outburst state.During the episode,the InsightHXMT satellite carried out a long observation that lasted for 20 days.More than 300 bursts were detected,and ...
supported by the National Natural Science Foundation of China(Nos.U1938201 and 12373042)。
GRB 200612A could be classified as an ultralong gamma-ray burst due to its prompt emission lasting up to~1020 s and the true timescale of the central engine activity t_(burst)≥4×10^(4) s.The late X-ray light curve w...
supported by the National Key R&D Program of China(2021YFA0718500)from the Minister of Science and Technology of China(MOST);supports from the National Natural Science Foundation of China under grants 12173103,12003028,U2038101,U2038102 and 11733009;supported by International Partnership Program of Chinese Academy of Sciences(grant No.113111KYSB20190020);the National SKA Program of China(2022SKA0130100);the China Manned Spaced Project(CMS-CSST-2021-B11)。
Fast radio bursts(FRBs)are short pulses observed in radio frequencies usually originating from cosmological distances.The discovery of FRB 200428 and its X-ray counterpart from the Galactic magnetar SGR J1935+2154sugg...