activity
20032025
most citedThe single degenerate channel for the progenitors of type Ia supernovae

421 citations · 778 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2025★ 1 cited

Scientific Objectives of the Xue-shan-mu-chang 15-meter Submillimeter Telescope

XSMT Project Collaboration Group, Yiping Ao, Jin Chang +48

Submillimeter astronomy is poised to revolutionize our understanding of the Universe by revealing cosmic phenomena hidden from optical and near-infrared observations, particularly…

astro-ph.HE2017★ 12 cited

A Polarization Sequence for Type Ia Supernovae?

Xiangcun Meng, Jujia Zhang, Zhanwen Han

Early polarization observations on Type Ia supernovae (SNe Ia) may reveal the geometry of supernova ejecta, and then put constraints on their explosion mechanism and their progenit…

astro-ph.SR2014★ 45 cited

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…

astro-ph.SR2009★ 23 cited

The masses of hot subdwarfs

X. Zhang, X. Chen, Z. Han

Masses are a fundamental parameter, but they are not well known for most hot subdwarfs. In general, the mass of a hot subdwarf is derived with asteroseismology or dynamical methods…

astro-ph.GA2009★ 53 cited

Ultra-cool dwarfs: new discoveries, proper motions, and improved spectral typing from SDSS and 2MASS photometric colors

Z. H. Zhang, R. S. Pokorny, H. R. A. Jones +6

Aims. We try to identify ultra-cool dwarfs from the seventh Data Release of the Sloan Digital Sky Survey (SDSS DR7) with SDSS i-z and r-z colors. We also obtain proper motion data…

astro-ph2008

The single degenerate channel for the progenitor of type Ia supernovae

Xiangcun Meng, Xuefei Chen, Zhanwen Han

We have carried out a detailed study of the single-degenerate channel for the progenitors of type Ia supernovae (SNe Ia). In the model, a carbon-oxygen white dwarf (CO WD) accretes…