54 citations · 253 across the 14 of their papers we have counts for
16 papers
A Unified Solution to the Low-Mass X-ray Binary Diversity Puzzle: Saturated Magnetic Braking Coupled with Irradiation-Driven Winds
Zhu-Ling Deng, Xiang-Dong Li, Bo Wang +4
The standard magnetic braking (MB) model has long failed to explain key properties of low-mass X-ray binaries (LMXBs)---including their accretion rates, the formation of ultracompa…
The double white dwarf merger model for the progenitors of SN 2021yfj-like events
Dongdong Liu, Chengyuan Wu, Takashi J. Moriya +4
Context. Recently, a new class of supernovae with prominent narrow emission features of Si, S and Ar has been reported, i.e. SN 2021yfj-like events (SNe Ien). Their progenitor orig…
Ultra-compact X-ray Binaries: A Review
Bo Wang, Dongdong Liu, Yunlang Guo +3
Ultra-compact X-ray binaries (UCXBs) are a subclass of low-mass X-ray binaries (LMXBs) characterized by ultra-short orbital periods, typically less than min. They consist…
A born ultramassive white dwarf-hot subdwarf super-Chandrasekhar candidate
Changqing Luo, Jiao Li, Chuanjie Zheng +16
Although supernovae is a well-known endpoint of an accreting white dwarf, alternative theoretical possibilities has been discussing broadly, such as the accretion-induced collapse…
Formation of millisecond pulsars with wide orbits
Bo Wang, Dongdong Liu, Yunlang Guo +4
Millisecond pulsars (MSPs) are a kind of radio pulsars with short spin periods, playing a key role in many aspects of stellar astrophysics. In recent years, some more MSPs with wid…
The progenitors of Type Ia supernovae with asymptotic giant branch donors
Luhan Li, Dongdong Liu, Bo Wang
Type Ia supernovae (SNe Ia) are among the most energetic events in the Universe. They are excellent cosmological distance indicators due to the remarkable homogeneity of their ligh…
Evolving ONe WD+He WD systems to ultra-compact X-ray binaries
Dongdong Liu, Bo Wang
It has been proposed that accretion-induced collapse (AIC) of massive white dwarfs (WDs) is an indispensable path for the formation of neutron star (NS) binaries. Although there ar…
The fractions of post-binary-interaction stars and evolved blue straggler stars on the red giant branch of globular clusters
Dandan Wei, Bo Wang, Hailiang Chen +4
The red giant branch (RGB) of globular clusters (GCs) is home to some exotic stars, which may provide clues on the formation of multiple stellar populations in GCs. It is well know…
The double-degenerate model for the progenitors of type Ia supernovae
Dongdong Liu, Bo Wang, Zhanwen Han
The double-degenerate (DD) model, involving the merging of massive double carbon-oxygen white dwarfs (CO WDs) driven by gravitational wave radiation, is one of the classical pathwa…
The progenitors of type Ia supernovae in the semidetached binaries with red giant donors
Dongdong Liu, Bo Wang, Hongwei Ge +2
Context. The companions of the exploding carbon-oxygen white dwarfs (CO WDs) for producing type Ia supernovae (SNe Ia) are still not conclusively confirmed. A red-giant (RG) star h…
The core-degenerate scenario for the progenitors of type Ia supernovae
Bo Wang, Weihong Zhou, Zhaoyu Zuo +5
The origin of the progenitors of type Ia supernovae (SNe Ia) is still uncertain. The core-degenerate (CD) scenario has been proposed as an alternative way for the production of SNe…
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…
Is the X-ray pulsating companion of HD 49798 a possible type Ia supernova progenitor?
Dong-Dong Liu, Wei-Hong Zhou, Cheng-Yuan Wu +1
HD 49798 (a hydrogen depleted subdwarf O6 star) with its massive white dwarf (WD) companion has been suggested to be a progenitor candidate of type Ia supernovae (SNe Ia). However,…
Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors
Weihong Zhou, Bo Wang, Xiangcun Meng +2
The core-degenerate (CD) scenario has been suggested to be a possible progenitor model of type Ia supernovae (SNe Ia), in which a carbon-oxygen white dwarf (CO WD) merges with the…
The hybrid CONe WD + He star scenario for the progenitors of type Ia supernovae
Bo Wang, Xiangcun Meng, Dongdong Liu +2
The hybrid CONe white dwarfs (WDs) have been suggested to be possible progenitors of type Ia supernovae (SNe Ia). In this article, we systematically studied the hybrid CONe WD + He…
On the evolution of rotating accreting white dwarfs and type Ia supernovae
Bo Wang, Stephen Justham, Zhengwei Liu +3
The potential importance of the angular momentum which is gained by accreting white dwarfs (WDs) has been increasingly recognized in the context of type Ia supernova (SN Ia) single…