IMBHs in globular clusters: Accretion rate correlations with cluster parameters

por Pepe, C., Pellizza, L.J., Castellani M., Ventura P., Charbonnel C., Di Criscienzo M.

Grids of stellar models with rotation : I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)

por Ekström, S., Georgy, C., Eggenberger, P., Meynet, G., Mowlavi, N., Wyttenbach, A., Granada, Anahí, Decressin, T., Hirschi, R., Frischknecht, U., Charbonnel, C., Maeder, A.
Publicado 2012