Eso1141b
The UV–Metallicity Characteristics of UCDs/IGCs in the Fornax Cluster
Run your own GALEV model - an introduction
Surprising Science
Research School of Astronomy & AstrophysicsSlide 1 SkyMapper SkyMapper and the Stromlo Southern Sky Survey Stefan Keller, Brian Schmidt, Paul Francis and.
The Age-Metallicity-Velocity relation in the nearby disk Borja Anguiano Astrophysikalisches Institut Potsdam (AIP) K. Freeman (ANU), E. Wylie de Boer (ANU),
Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen.
CRyA Mass Loss Return from Stars to Galaxies, STScI, 30 March 2012 Self-consistent mass-loss in stellar population synthesis models Rosa A. González-Lópezlira.
AGB POPULATION IN GALAXIES WHY? Up to 80% of the K-band luminosity in a 1 Gyr old simple stellar population comes from AGB stars High redshift galaxies.
© 2005 Pearson Education Inc., publishing as Addison-Wesley The Fate of our Sun & The Origin of Atoms The Death of our Sun and other Stars Nuclear Reactions.
Observing galaxy cluster simulations with an X-ray telescope Elena Rasia Department of Physics, University of Michigan Chandra Fellows Symposium Harvard-Smithsonian.
Claudia Lagos U. 8 Abril 2008 Seminario de Astrofísica “Semi-analytic galaxies (SAG) model: results on BH and galaxy population” Claudia Lagos (PUC, Chile)
