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Andr\'e Maeder

Identifiers

  • name variant Andr\'e Maeder 0.60 · backfill

Papers (32)

  1. Pre-supernova mixing in CEMP-no source stars astro-ph.SR · 2017 · author #4
  2. Massive stars, successes and challenges astro-ph.SR · 2017 · author #2
  3. Massive star formation by accretion II. Rotation: how to circumvent the angular momentum barrier? astro-ph.SR · 2017 · author #4
  4. Constraints on CEMP-no progenitors from nuclear astrophysics astro-ph.SR · 2016 · author #2
  5. Massive star formation by accretion I. Disc accretion astro-ph.SR · 2015 · author #4
  6. $s$-process production in rotating massive stars at solar and low metallicities astro-ph.SR · 2015 · author #4
  7. Clues about the first stars from CEMP-no stars astro-ph.SR · 2015 · author #3
  8. Populations of rotating stars III. SYCLIST, the new Geneva Population Synthesis code astro-ph.SR · 2014 · author #8
  9. Evolution of surface CNO abundances in massive stars astro-ph.SR · 2014 · author #1
  10. Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002 astro-ph.SR · 2013 · author #6
  11. The thermohaline, Richardson, Rayleigh-Taylor, Solberg-Hoiland, and GSF criteria in rotating stars astro-ph.SR · 2013 · author #1
  12. Populations of rotating stars. - I. Models from 1.7 to 15 Msun at Z = 0.014, 0.006, and 0.002 with {\Omega}/{\Omega}crit between 0 and 1 astro-ph.SR · 2013 · author #7
  13. Models of rotating massive stars: impacts of various prescriptions astro-ph.SR · 2013 · author #3
  14. Grids of stellar models with rotation II. WR populations and supernovae/GRB progenitors at Z = 0.014 astro-ph.SR · 2012 · author #8
  15. On the Eddington limit and WR Stars astro-ph.SR · 2012 · author #1
  16. Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014) astro-ph.SR · 2011 · author #12
  17. Effects of anisotropic winds on massive stars evolution astro-ph.SR · 2010 · author #3
  18. Massive stellar models: rotational evolution, metallicity effects astro-ph.SR · 2010 · author #4
  19. The different progenitors of type Ib, Ic SNe, and of GRB astro-ph.SR · 2009 · author #5
  20. The basic role of magnetic field in stellar evolution astro-ph · 2008 · author #1
  21. Wind anisotropy and stellar evolution astro-ph · 2008 · author #3
  22. Can very massive stars avoid Pair-Instability Supernovae? astro-ph · 2008 · author #3
  23. Convective envelopes in rotating OB stars astro-ph · 2008 · author #1
  24. CNO production in first generation stars astro-ph · 2006 · author #3
  25. On the Origin of the High Helium Sequence in $\omega$ Centauri astro-ph · 2006 · author #1
  26. Initial conditions for reaching the critical velocity astro-ph · 2006 · author #3
  27. Effects of Rotation on Mass Loss for Population III stars astro-ph · 2005 · author #3
  28. Stellar evolution with rotation and magnetic fields:III: The interplay of circulation and dynamo astro-ph · 2005 · author #1
  29. Chemical Abundances and Yields from Massive Stars astro-ph · 2004 · author #1
  30. Evolution at very low and zero Z astro-ph · 2004 · author #2
  31. Evolution of the Most Massive Stars astro-ph · 2004 · author #1
  32. Stellar rotation: Evidence for a large horizontal turbulence and its effects on evolution astro-ph · 2003 · author #1

Mentions

  • 1203.5243 #8 · backfill · confidence 0.70 Andr\'e Maeder
  • 1201.5013 #1 · backfill · confidence 0.70 Andr\'e Maeder
  • 1110.5049 #12 · backfill · confidence 0.70 Andr\'e Maeder
  • 1011.6581 #3 · backfill · confidence 0.70 Andr\'e Maeder
  • 1010.3838 #4 · backfill · confidence 0.70 Andr\'e Maeder
  • 0906.2284 #5 · backfill · confidence 0.70 Andr\'e Maeder
  • 0812.2764 #1 · backfill · confidence 0.70 Andr\'e Maeder
  • 0807.5061 #3 · backfill · confidence 0.70 Andr\'e Maeder
  • 0801.3397 #3 · backfill · confidence 0.70 Andr\'e Maeder
  • 0801.1018 #1 · backfill · confidence 0.70 Andr\'e Maeder

Frequent Coauthors