activity
20092023
most citedHigh Fill-Out, Extreme Mass Ratio Overcontact Binary Systems. X. The new discovered binary XY Leonis Minoris

35 citations · 98 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2023

White-light superflare and long-term activity of the nearby M7 type binary EI~Cnc observed with GWAC system

Hua-Li Li, Jing Wang, Li-Ping Xin +14

Stellar white-light flares are believed to play an essential role on the physical and chemical properties of the atmosphere of the surrounding exoplanets. Here we report an optical…

astro-ph.SR2023★ 12 cited

Photometric observations of flares on AD Leo from GWAC-F30 and TESS

Jian-Ying Bai, Jing Wang, Hua-Li Li +4

We observed active M dwarf star AD Leo for 146 hr in photometry by GWAC-F30 and also analyzed 528-hr photometric data of the star from TESS. A total of 9 and 70 flares are detected…

astro-ph.HE2023★ 17 cited

Prompt-to-afterglow transition of optical emission in a long gamma-ray burst consistent with a fireball

Liping Xin, Xuhui Han, Huali Li +19

Long gamma-ray bursts (GRBs), which signify the end-life collapsing of very massive stars, are produced by extremely relativistic jets colliding into circumstellar medium. Huge ene…

astro-ph.SR2023★ 4 cited

A huge-amplitude white-light superflare on a L0 brown dwarf discovered by GWAC survey

Li-Ping Xin, Hua-li Li, Jing Wang +21

White-light superflares from ultra cool stars are thought to be resulted from magnetic reconnection, but the magnetic dynamics in a fully convective star is not clear yet. In this…

astro-ph.IM2021★ 24 cited

An Automatic Observation Management System of the GWAC Network I: System Architecture and Workflow

Xuhui Han, Yujie Xiao, PinPin Zhang +21

The GWAC-N is an observation network composed of multi-aperture and multi-field of view robotic optical telescopes. The main instruments are the GWAC-A. Besides, several robotic op…

astro-ph.SR2011★ 35 cited

High Fill-Out, Extreme Mass Ratio Overcontact Binary Systems. X. The new discovered binary XY Leonis Minoris

S. -B. Qian, L. Liu, L. -Y. Zhu +3

The new discovered short-period close binary star, XY LMi, was monitored photometrically since 2006. It is shown that the light curves are typical EW-type and show complete eclipse…