287 citations
- Tiangong UniversityCN40 papers
- Inner Mongolia University for NationalitiesCN26 papers
- Beijing Normal UniversityCN21 papers
- Chinese Academy of SciencesCN18 papers
- National Astronomical ObservatoriesCN12 papers
- Henan Normal UniversityCN8 papers
- Beijing University of Posts and TelecommunicationsCN7 papers
- Chongqing Normal UniversityCN7 papers
- Beijing Institute of TechnologyCN6 papers
- Dali UniversityCN6 papers
- Zhoukou Normal UniversityCN6 papers
- Institute of Applied Physics and Computational MathematicsCN5 papers
26 papers · 1 filter
Asteroseismic analysis of Kepler target KIC 2837475
Wuming Yang, Zhijia Tian, Shaolan Bi +3
The ratios and of small to large separations of KIC 2837475 primarily exhibit an increase behavior in the observed frequency range. The calculations indicate that…
Asteroseismic analysis of the CoRoT target HD49933
Zhie Liu, Wuming Yang, Shaolan Bi +9
The frequency ratios and of HD 49933 exhibit an increase at high frequencies. This behavior also exists in the ratios of other stars, which is considered to result from the low sig…
Constraining the spin-down timescale of the white-dwarf progenitors of Type Ia supernovae
Xiangcun Meng, Philipp Podsiadlowski
Justham (2011) and DiStefano et al.\ (2011) proposed that the white-dwarf progenitor of a Type Ia supernova (SN Ia) may have to spin down before it can explode. As the white dwarf…
The effects of rotation on the main-sequence turnoff of intermediate-age massive star clusters
Wuming Yang, Shaolan Bi, Xiangcun Meng +1
The double or extended main-sequence turnoffs (MSTOs) in the color-magnitude diagram (CMD) of intermediate-age massive star clusters in the Large Magellanic Cloud are generally int…
Evolution of rotational velocities of A-type stars
Wuming Yang, Shaolan Bi, Xiangcun Meng +1
It was found that the equatorial velocity of A-type stars undergoes an acceleration in the first third of the main sequence (MS) stage, but the velocity decreases as if the stars w…
Grids of rotating stellar models with masses between 1.0 and 3.0 Msun
Wuming Yang, Shaolan Bi, Xiangcun Meng
We calculated a grid of evolutionary tracks of rotating models with masses between 1.0 and 3.0 and a resolution , which can be used to study t…