Shuai Zhang

GRB 140903A, a short duration $γ -$ ray burst (SGRB) detected by {\it Swift}, is characterized by its long-lasting radio emission among SGRBs. In addition to the $\sim 1 0^{6}$ s radi…

astro-ph.HE2016★ 23 cited

Evaluating the bulk Lorentz factors of outflow material: lessons learned from the extremely-energetic outburst GRB 160625B

Yuan-Zhu Wang, Hao Wang, Shuai Zhang +6

GRB 160625B is an extremely-bright outburst with well-monitored afterglow emission. The geometry-corrected energy is high up to $\sim 5.2 \times 1 0^{52}$ erg or even $\sim 8\times 10…

astro-ph.GA2016★ 26 cited

Molecular clouds and star formation toward the Galactic plane within 216.25 $^{o} \leq$ l $\leq$ 218.75 $^{o}$ and $-$ 0.75 $^{o} \leq$ b $\leq$ 1.25 $^{o}$

Y. Gong, R. Q. Mao, M. Fang +9

As a part of the Milky Way Imaging Scroll Painting (MWISP) survey, we performed a simultaneous 12CO(1-0), 13CO(1-0), C18O(1-0) mapping toward molecular clouds in a region encompass…

The interpretation of the multi-wavelength afterglow emission of short GRB 140903A

Evaluating the bulk Lorentz factors of outflow material: lessons learned from the extremely-energetic outburst GRB 160625B

Molecular clouds and star formation toward the Galactic plane within 216.25o≤ l ≤218.75o and −0.75o≤ b ≤1.25o

Molecular clouds and star formation toward the Galactic plane within 216.25 $^{o} \leq$ l $\leq$ 218.75 $^{o}$ and $-$ 0.75 $^{o} \leq$ b $\leq$ 1.25 $^{o}$