activity
20122016
most citedAsteroseismic Study on Cluster Distance Moduli for RGB Stars in NGC 6791 and NGC 6819

31 citations · 100 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2016★ 19 cited

New Insights for High-precision Asteroseismology: Acoustic Radius of KIC 6225718

Tao Wu, Yan Li

Asteroseismology is a powerful tool for probing stellar interiors and determining stellar fundamental parameters. In previous works, -minimization method is usually used to fi…

astro-ph.SR2015★ 22 cited

Numerical experiments on the detailed energy conversion and spectrum studies in a corona current sheet

Lei Ni, Jun Lin, Zhixing Mei +1

In this paper, we study the energy conversion and spectra in a corona current sheet by 2.5-dimensional MHD numerical simulations. Numerical results show that many Petschek-like fin…

astro-ph.SR2015★ 28 cited

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…

astro-ph.SR2014★ 31 cited

Asteroseismic Study on Cluster Distance Moduli for RGB Stars in NGC 6791 and NGC 6819

Tao Wu, Yan Li, Saskia Hekker

Stellar distance is an important basic parameter in stellar astrophysics. Stars in a cluster are thought to be formed coevally from the same interstellar cloud of gas and dust. The…

astro-ph.SR2013

Asteroseismology of DAV white dwarf stars and G29-38

Yan-Hui Chen, Yan Li

Asteroseismology is a powerful tool to detect the inner structure of stars. It is also widely used to study white dwarfs. In this paper, we discuss the asteroseismology work of DAV…

astro-ph.SR2012

A k-omega model for stellar turbulent convection

Yan Li

Both observations and numerical simulations show that stellar convective motions are composed of semi-regular flows of convective rolling cells and the fully developed turbulence.…