activity
20152026
most citedHigh-precision asteroseismology in Slowly Pulsating B star: HD 50230

34 citations · 120 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2026

Asteroseismic Analysis of a Red Giant KIC 9145955 by Including the Small-scale Magnetic Fields in the Atmosphere

Yuetong Wang, Guifang Lin, Yan Li +2

Recent convincing evidence is found within asteroseismology that suggests the magnetic fields exist in three red giants. Research on small-scale magnetic fields in the Sun and HD 4…

astro-ph.SR2024★ 3 cited

Exploring the small-scale magnetic fields of the solar analog KIC 8006161 using asteroseismology

Lin Guifang, Li Yan, Su Jie +2

The magnetic field is a significant and universal physical phenomenon in modern astrophysics. Small-scale magnetic fields are very important in the stellar atmosphere. They are ubi…

astro-ph.SR2023★ 7 cited

Asteroseismic investigation on KIC 10526294 to probe convective core overshoot mixing

Qian-Sheng Zhang, Li Yan, Wu Tao +1

In the overshoot mixing model with an exponentially decreasing diffusion coefficient, the initial value of the diffusion coefficient plays a crucial role. According to the turbulen…

astro-ph.SR2019★ 34 cited

High-precision asteroseismology in Slowly Pulsating B star: HD 50230

Tao Wu, Yan Li

SPB star HD 50230, in fact a hybrid B-type pulsator, has been observed by CoRoT least 137 days. A nearly equidistant period spacing pattern are found among 8 modes which are extrac…

astro-ph.SR2018★ 14 cited

A new C-D-like diagram for SPB stars: The variations of period spacing as a signature of evolutionary status

Tao Wu, Yan Li, Zhen-min Deng

The Slowly Pulsating B-type (SPB) stars are the upper main-sequence stars on the HR diagram. Their oscillations are high-order, low-degree g-mode and can be used to probe the struc…

astro-ph.SR2018★ 31 cited

Which evolutionary status does the Blue Large-Amplitude Pulsators stay at?

Tao Wu, Yan Li

Asteroseismology is a very useful tool for exploring the stellar interiors and evolutionary status and for determining stellar fundamental parameters, such as stellar mass, radius,…

astro-ph.SR2018★ 10 cited

Frequency identification and asteroseismic analysis of the red giant KIC 9145955: fundamental parameters and helium core size

Xinyi Zhang, Tao Wu, Yan Li

We have analyzed 18 quarters of long-cadence data of KIC 9145955 provided by \emph{Kepler}, and extracted 61 oscillation frequencies from these high precision photometric data. The…

physics.optics2016★ 20 cited

Background-free coherent anti-stokes Raman spectroscopy and microscopy by dual-soliton pulse generation

Kun Chen, Tao Wu, Haoyun Wei +1

We propose an all-fiber-generated dual-soliton pulses based scheme for the background-free detection of coherent anti-Stokes Raman spectroscopy under the spectral focusing mechanis…

astro-ph.SR2015★ 1 cited

The Asteroseismology of ZZ Ceti star GD1212

Lin Guifang, Li Yan, Su Jie

The ZZ Ceti star GD 1212 was detected to have 19 independent modes from the two-wheel-controlled Kepler Spacecraft in 2014. By asymptotic analysis, we identify most of pulsation mo…