G.Meynet

Identifiers

• name variant G.Meynet 0.60 · backfill

Papers (2)

1. How did globular clusters lose their gas? astro-ph.GA · 2012 · author #4
2. Grids of stellar models. VIII. From 0.4 to 1.0 Msun at Z=0.020 and Z=0.001, with the MHD equation of state astro-ph · 1998 · author #6

Mentions

• 1211.0143 #4 · backfill · confidence 0.70 G.Meynet

Frequent Coauthors

• C.Charbonnel 2 shared papers
• A.Maeder 1 shared papers
• D.Schaerer 1 shared papers
• M.Krause 1 shared papers
• N.Mowlavi 1 shared papers
• N.Prantzos 1 shared papers
• P.A.Bernasconi 1 shared papers
• R.Diehl 1 shared papers
• T.Decressin 1 shared papers
• W.Dappen 1 shared papers