The Gradients in the 47 Tuc Red Giant Branch Bump and Horizontal Branch are Consistent With a Centrally-Concentrated, Helium-Enriched Second Stellar Generation Authors: D. M. Nataf, A. Gould, M.H. Pinsonneault, P.B. Stetson

Radial distribution of stars, gas and dust in SINGS galaxies. III. Modeling the evolution of the stellar component in galaxy disks Authors: J. C. Muņoz-Mateos (1,2), S. Boissier (3), A. Gil de Paz (2), J. Zamorano (2), R. C. Kennicutt Jr. (4,5), J. Moustakas (6), N. Prantzos (7), J. Gallego

Open Issues on the Synthesis of Evolved Stellar Populations at Ultraviolet Wavelengths Authors: Miguel Chavez (1), Emanuele Bertone (1) ((1) INAOE, Puebla, Mexico)

Modeling the formation and evolution of star cluster populations in galaxy simulations Authors: J. M. Diederik Kruijssen, F. Inti Pelupessy, Henny J. G. L. M. Lamers, Simon F. Portegies Zwart, Vincent Icke

Radial distribution of stars, gas and dust in SINGS galaxies. III. Modeling the evolution of the stellar component in galaxy disks Authors: J. C. Muņoz-Mateos (1,2), S. Boissier (3), A. Gil de Paz (2), J. Zamorano (2), R. C. Kennicutt Jr. (4,5), J. Moustakas (6), N. Prantzos (7), J. Gallego (2) ((1) National Radio Astronomy Observatory, (2)