66 citations · 157 across the 18 of their papers we have counts for
18 papers
Magneto hydrodynamic simulations of the supernova remnant G1.9+0.3
Shaobo Zhang, Wenwu Tian, Mengfei Zhang +2
The youngest Galactic supernova remnant G1.9+0.3 shows a discrete feature between its radio and X-ray morphologies. The observed radio morphology features a single maximum in the n…
TESS Timings of 31 Hot Jupiters with Ephemeris Uncertainties
Su-Su Shan, Fan Yang, You-Jun Lu +8
A precise transit ephemeris serves as the premise for follow-up exoplanet observations. We compare TESS Objects of Interest (TOI) transit timings of 262 hot Jupiters with the archi…
X-ray Spectra from Plasmas with High-Energy Electrons: kappa-distributions and e-e Bremsstrahlung
Xiaohong Cui, Adam R. Foster, Takayuki Yuasa +1
Shocks, turbulence and winds all influence the electron velocity distribution in hot plasmas, exciting lower-energy electrons and generating a high-energy (typically power-law) tai…
Constraining External Reverse Shock Physics of GRBs from ROTSE-III Limits
Xiao-Hong Cui, Yuan-Chuan Zou, Jun-Jie Wei +2
Assuming that the early optical emission is dominated by the external reverse shock (RS) in the standard model of gamma-ray bursts (GRBs), we intend to constrain RS models with the…
Searching for the Time Variation in Supernova Remnant RX J1713.7-3946
Aytap Sezer, Ryo Yamazaki, Xiaohong Cui +2
Supernova Remnant RX J1713.7-3946 emits synchrotron X-rays and very high energy -rays. Recently, thermal X-ray line emission is detected from ejecta plasma. CO and HI observatio…
Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs
Bo Wang, Yan Li, Xin Ma +3
Supernovae of type Ia (SNe Ia) are believed to be thermonuclear explosions of carbon-oxygen white dwarfs (CO WDs). However, the mass accretion process onto CO WDs is still not comp…