24 citations · 58 across the 7 of their papers we have counts for
7 papers
A Path to Constraints on Common Envelope Ejection in Massive Binaries: Full Evolutionary Reconstruction of Three Black Hole X-ray Binaries
Zhenwei Li, Dandan Wei, Shi Jia +6
The massive binary common envelope (CE) phase plays a pivotal role in the formation of close black hole/neutron star (BH/NS) binaries, yet significant uncertainties remain in our u…
Ohmic dissipation during the formation of super-Earth
Shi Jia, Wei Zhong, Cong Yu
Super-Earth population, as one of the representatives of exoplanets, plays an important role in constraining the planet formation theories. According to the prediction from core-ac…
Three New Late-type Hypervelocity Star Candidates from Gaia DR2 with Refined Selection Criteria
Jiao Li, Shi Jia, Yan Gao +6
Several dozen hypervelocity star (HVS) candidates have been reported based on the second data release of Gaia (Gaia DR2). However, it has been proven that the radial velocities of…
High Velocity Runaway Binaries from Supernovae in Triple Systems
Yan Gao, Jiao Li, Shi Jia
Recent studies on hypervelocity stars (HVSs) have generated a need to understand the high velocity limits of binary systems. If runaway binary systems with high movement speeds wel…
Disruption of a planet spiralling into its host star
Shi Jia, H. C. Spruit
The processes leading deformation and destruction of planets spiraling into the convective envelope of their host stars are described. The planet is compressed by the ram pressure,…
Instability of mass transfer in a planet-star system
Shi Jia, H. C. Spruit
We show that the angular momentum exchange mechanism governing the evolution of mass transferring binary stars does not apply to Roche-lobe filling planets, because most of the ang…
Double-detonation explosions as progenitors of type Iax supernovae
Bo Wang, Stephen Justham, Zhanwen Han
It has recently been proposed that one sub-class of type Ia supernovae (SNe Ia) is sufficiently both distinct and common to be classified separately from the bulk of SNe Ia, with a…