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Wuming Yang

Identifiers

  • name variant Wuming Yang 0.60 · backfill

Papers (33)

  1. Rotating Solar Models with Low Metal Abundances as Good as Those with High Metal Abundances astro-ph.SR · 2019 · author #1
  2. Estimating The Mean Linewidth And Lifetime of Solar-like Oscillations of Stars astro-ph.SR · 2018 · author #1
  3. The Effects of Binary Stars on the Color-Magnitude Diagrams of Young-Age Massive Star Clusters astro-ph.SR · 2018 · author #1
  4. Binary Star Fractions from the LAMOST DR4 astro-ph.SR · 2018 · author #15
  5. The effects of the overshooting of the convective core on main-sequence turnoffs of young- and intermediate-age star clusters astro-ph.SR · 2017 · author #1
  6. Estimate the radius of the convective core of main-sequence stars from observed oscillation frequencies astro-ph.SR · 2016 · author #1
  7. Solar models with new low-metal abundances astro-ph.SR · 2016 · author #1
  8. Asteroseismic analysis of Kepler target KIC 2837475 astro-ph.SR · 2015 · author #1
  9. A Large Convective-Core Overshoot in \textit{Kepler} Target KIC 11081729 astro-ph.SR · 2015 · author #1
  10. Asteroseismic analysis of solar-mass subgiants KIC 6442183 and KIC 11137075 observed by Kepler astro-ph.SR · 2015 · author #4
  11. Exploring the sources of p-mode frequency shifts in the CoRoT target HD 49933 astro-ph.SR · 2014 · author #3
  12. The effects of rotation on the main-sequence turnoff of intermediate-age massive star clusters astro-ph.SR · 2013 · author #1
  13. Evolution of rotational velocities of A-type stars astro-ph.SR · 2013 · author #1
  14. Grids of rotating stellar models with masses between 1.0 and 3.0 Msun astro-ph.SR · 2012 · author #1
  15. The birth rate of supernovae from double-degenerate and core-degenerate systems astro-ph.SR · 2012 · author #2
  16. Characteristics of solar-like oscillations of secondary red clump stars astro-ph.SR · 2012 · author #1
  17. The companion properties of SNe Ia from the single degenerate model astro-ph.SR · 2011 · author #2
  18. The effect of metallicity on the delay-time distribution of type Ia supernova astro-ph.SR · 2011 · author #3
  19. The correlation between C/O ratio, metallicity and the initial WD mass for SNe Ia astro-ph.SR · 2011 · author #2
  20. Binary population synthesis study on supersoft X-ray phase of single degenerate type Ia supernova progenitors astro-ph.SR · 2011 · author #2
  21. Solar Models with Revised Abundance astro-ph.SR · 2011 · author #4
  22. The Contributions of Interactive Binary Stars to Double Main Sequence Turn-Offs and Dual Red Clump of Intermediate-Age Star Clusters astro-ph.SR · 2011 · author #1
  23. Characteristics of solar-like oscillations of clusters simulated by stellar population synthesis astro-ph.SR · 2011 · author #1
  24. The birth rate of subluminous and overluminous type Ia supernovae astro-ph.SR · 2010 · author #3
  25. The effects of stellar population synthesis on the distributions of the asteroseismic observables {\nu}_max and {\Delta}{\nu} of red-clump stars astro-ph.SR · 2010 · author #1
  26. The envelope mass of red giant donors in Type Ia supernova progenitors astro-ph.SR · 2010 · author #2
  27. WD + MS systems as the progenitor of SNe Ia astro-ph.SR · 2009 · author #2
  28. Frequency separation variations of the solar low-degree p-modes astro-ph.SR · 2009 · author #1
  29. A comprehensive progenitor model for SNe Ia astro-ph.SR · 2009 · author #2
  30. Is SN 2006X from a WD + MS system with optically thick wind? astro-ph.SR · 2009 · author #2
  31. Companion Stars of Type Ia supernovae with different metallicities astro-ph.SR · 2009 · author #2
  32. WD+MS Systems as the Progenitors of Type Ia Supernovae with Different Metallicities astro-ph.SR · 2009 · author #2
  33. Rotation profiles of solar-like stars with magnetic fields astro-ph · 2008 · author #1

Mentions

  • 1402.4925 #3 · backfill · confidence 0.70 Wuming Yang
  • 1304.5865 #1 · backfill · confidence 0.70 Wuming Yang
  • 1302.0448 #1 · backfill · confidence 0.70 Wuming Yang
  • 1212.1511 #1 · backfill · confidence 0.70 Wuming Yang
  • 1205.2452 #2 · backfill · confidence 0.70 Wuming Yang
  • 1202.2017 #1 · backfill · confidence 0.70 Wuming Yang
  • 1112.0082 #2 · backfill · confidence 0.70 Wuming Yang
  • 1105.5265 #3 · backfill · confidence 0.70 Wuming Yang
  • 1105.2860 #2 · backfill · confidence 0.70 Wuming Yang
  • 1105.0754 #2 · backfill · confidence 0.70 Wuming Yang
  • 1104.1032 #4 · backfill · confidence 0.70 Wuming Yang
  • 1103.3128 #1 · backfill · confidence 0.70 Wuming Yang
  • 1102.1082 #1 · backfill · confidence 0.70 Wuming Yang
  • 1010.5293 #3 · backfill · confidence 0.70 Wuming Yang
  • 1007.1752 #1 · backfill · confidence 0.70 Wuming Yang
  • 1003.2659 #2 · backfill · confidence 0.70 Wuming Yang
  • 0912.0804 #2 · backfill · confidence 0.70 Wuming Yang
  • 0911.1531 #1 · backfill · confidence 0.70 Wuming Yang
  • 0910.4992 #2 · backfill · confidence 0.70 Wuming Yang
  • 0910.1915 #2 · backfill · confidence 0.70 Wuming Yang
  • 0909.2167 #2 · backfill · confidence 0.70 Wuming Yang
  • 0908.2480 #2 · backfill · confidence 0.70 Wuming Yang
  • 0805.2323 #1 · backfill · confidence 0.70 Wuming Yang

Frequent Coauthors