The masses of Population III stars
Copyright policy ) J. C. N. de Araujo; R. Opher;
The masses of Population III stars
La formation de proto-etoiles de Population III est etudiee en suivant l'hypothese que la permanence des fluctuations de masse 10-1000 M○. apres l'ere de recombinaison peut etre importante dans la fragmentation des nuages massifs de masse ∼M J pour former des etoiles de population III, ou M J est la masse de Jeans pendant l'ere de recombinaison
- Universidade de São Paulo Brazil
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