output
20162026
most citedATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XV. Steady Accretion from Global Collapse to Core Feeding in Massive Hub-filament System SDC335

71 citations

Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR2023★ 8 cited

Properties and Asteroseismological analysis of a new ZZ ceti discovered by TMTS

Jincheng Guo, Yanhui Chen, Xiaofeng Wang +24

Tsinghua university-Ma Huateng Telescope for Survey (TMTS) aims to discover rapidly evolving transients by monitoring the northern sky. The TMTS catalog is cross-matched with the w…

astro-ph.SR2022★ 8 cited

Asteroseismology of the DAV star L19-2

Yanhui Chen

L19-2 is a DAV star, which has been intermittently observed from 1976 to 2013. Five independent pulsation modes of 350\,s, 192\,s, 143\,s, 118\,s, and 113\,s are identified. The fi…

astro-ph.SR2022★ 6 cited

The preliminary statistical analysis of LAMOST DR8 low resolution AFGK stars

Yan hui Chen, Guang Wei Li, Hong Shu

We download the LAMOST DR8 low resolution catalog 6,478,063 AFGK tpye stars and plot the figures of effective temperature, gravitational acceleration, and metal abundance. Some sma…

astro-ph.SR2021★ 17 cited

EPIC 228782059: Asteroseismology of what could be the coolest pulsating helium-atmosphere white dwarf (DBV) known?

R. M. Duan, W. Zong, J. -N. Fu +5

We present analysis of a new pulsating helium-atmosphere (DB) white dwarf, EPIC~228782059, discovered from 55.1~days of {\em K2} photometry. The long duration, high quality light c…

astro-ph.SR2020

Asteroseismology of the DAV star R808

Yanhui Chen, Hong Shu

The DAV star R808 was observed by 13 different telescopes for more than 170 hours in April 2008 on the WET run XCOV26. 25 independent pulsation frequencies were identified by this…

astro-ph.SR2020★ 2 cited

Application of a screened Coulomb potential in fitting the DAV star HS 0507+0434B

Yanhui Chen

We use \texttt{WDEC} to evolve grids of DAV star models adopting the element diffusion scheme with pure and screened Coulomb potential effect. The core compositions are thermonucle…

astro-ph.SR2019★ 1 cited

Asteroseismology of the DOV star PG 1159-035

Yanhui Chen

Grids of DOV star models are evolved by \texttt{WDEC} with fixed atmospheric constituent to the spectral values of = 50/33/17. The core compositions are from w…

astro-ph.SR2017★ 2 cited

The rate of period change in DAV stars

Y. H. Chen, C. Y. Ding, W. W. Na +1

Grids of DAV star models are evolved by \texttt{WDEC}, taking the element diffusion effect into account. The grid parameters are hydrogen mass log(), helium mass log($…

astro-ph.SR2016★ 11 cited

Exploring the helium core of the delta Scuti star CoRoT 102749568 with asteroseismology

Xinghao Chen, Yan Li, Guifang Lin +2

Based on regularities in rotational splittings, we seek possible multiplets for the observed frequencies of CoRoT 102749568. Twenty-one sets of multiplets are identified, including…

astro-ph.SR2016★ 3 cited

Asteroseismology of the DBV star CBS 114

Yanhui Chen

Asteroseismology is an unique and powerful tool to detect the internal structure of stars. CBS 114 is the sixth known pulsating DBV star. It was observed by Handler, Metcalfe, \& W…

astro-ph.SR2016★ 2 cited

The dispersion of period spacing for DAV stars

Yanhui Chen

Three groups of DAV star models are evolved with time-dependent element diffusion by \texttt{WDEC}. The core compositions of these models are directly from white dwarf models evolv…