supported by the National Basic Research Program of China (973 Program) (Grant No. 2015CB452804);the National Natural Science Foundation of China (Grant Nos. 41575064, 41875079, 91637102, 41475036, 91437215 and 41575047);the Basic Research Fund of CAMS (Grant No. 2017Y010)
Convective burst(CB) characteristics at distinct stages of a rapidly intensified Typhoon Mujigae(2015), are investigated based on a 72-h simulation. The spatial features show that almost all CB elements develop in the...
supported by the National Basic Research Program of China(973 Program,Grant No.2014CB845800);China Postdoctoral Science Foundation(Grant No.2017M612233);the National Natural Science Foundation of China(Grant Nos.11422325 and 11373022);the Excellent Youth Foundation of Jiangsu Province(BK 20140016)
X-ray flares are the most common phenomena in the afterglow phase of gamma-ray bursts (GRBs) in the Swift era, and are known as a canonical component in X-ray afterglows. In this work, we constrain the Lorentz facto...
supported by the National Natural Science Foundation of China(Grant Nos.50925104,11132006,51231005 and 51321003);the National Basic Research Program of China("973"Program)(Grant Nos.2010CB631003 and 2012CB619402);the support from the"111"Project of China(Grant No.B06025);JL also acknowledges the support by US National Science Foundation(Grant Nos.DMR-1240933 and DMR-1120901)
Mechanical tests on small-volume materials show that in addition to the usual attributes of strength and ductility, the controlla- bility of deformation would be crucial for the purpose of precise plastic shaping. In ...
supported by the National Natural Science Foundation of China(Grant Nos. 11033002 and J1210039);the National Basic Research Program of China (973 Program, Grant No. 2009CB824800)
The afterglow of GRB 081029 showed unusual behavior, with a signifi- cant rebrightening being observed at the optical wavelength at about 3000 s after the burst. One possible explanation is that the rebrightening resu...
Supported by the National Natural Science Foundation of China;supported by the National Basic Research Programof China (973 Program,2009CB824800);the China Postdoctoral Science Foundation funded project(No. 20110490590);the National Natural Science Foundation of China (Grant No. 111030262);the Foundation for the Authors of National Excellent Doctoral Dissertations of China
Observations imply that long "y-ray bursts (GRBs) originate from the explo- sions of massive stars, therefore they may occur in the molecular clouds where their progenitors were born. We show that the prompt optica...
the China Postdoctoral Science Foundation funded project (No. 20110490590);the National Natural Science Foundation of China under No.11103026;the National Basic Research Program of China (973 Program, 2009CB824800);Grant-in-Aid for Scientific Research on Priority Areas No. 19047004 by the Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan;Grant-in-Aid for Scientific Research (S) No. 19104006 by the Japan Society for the Promotion of Science (JSPS);the Grant-in-Aid for Young Scientists (B) No.19740139 by JSPS;the Grant-in-Aid for Scientific Research on Innovative Areas No. 21105509 by MEXT;Grant-in-Aid for JSPS Fellows from MEXT;the Grant-in-Aid for the Global COE Program "The Next Generation of Physics,Spun from Universality and Emergence" from MEXT
The spatial distribution of short Gamma-ray bursts (GRBs) in their host galaxies provides us with an opportunity to investigate their origins. Based on the currently observed distribution of short GRBs relative to the...
supported by the National Natural Science Foundation of China (Grant Nos. 11173011, 11003004,10703002, 11143001, 11133005 and 11103003);the National Basic Research Program of China(973 Program, 2009CB824800);Fundamental Research Funds for the Central Universities(HUST: 2011TS159)
We propose a two-component jet model consistent with the observations of several gamma ray bursts (GRBs) and active galactic nuclei (AGNs). The jet consists of inner and outer components, which are supposed to be ...
supported by the National Natural Science Foundation of China (Grants Nos.11025313, 10873002 and 11078008);National Basic Research Program of China (973 Program, Grant No.2009CB824800);Chinese Academy of Sciences (Grant KJCXZ-YW-T19);Guangxi SHI-BAI-QIAN project (Grant No.2007201);Guangxi Science Foundation (2010GXNSFC013011, 2011-135)
Swift GRB 100418A is a long burst at z = 0.624 without detection of any associated supernova (SN). Its light curves in both the prompt and afterglow phases are similar to GRB 060614, a nearby long GRB without an ass...
supported by the National Natural Science Foundation of China (Grant Nos.10625313 and 10473023);the National Basic Research Program of China (973 Program,Grant No.2009CB824800)
A long plateau phase and an amazing level of brightness have been observed in the X-ray afterglow of GRB 060729. This peculiar light curve is likely due to longterm energy injection in external shock. Here, we present...