Detection of optical surface brightness structures with magnitudes fainter than 30 mag/arcsec2 has remained elusive in current photometric deep surveys. We are...
What do RR Lyrae tell us about the formation of the Milky Way and M31 haloes?
RR Lyrae variables are old (>10 Gyr) stars and, as such, they are useful probes of the earliest events of star formation in galaxies (Bernard et al. 2008...
What do we find when nothing is found? A deep search for planetary nebulae at the outskirts of M33
Planetary nebulae (PNe) are excellent tracers of stellar populations with low surface brightness, and therefore provide a powerful method to detect and explore...
What do we really know about Spiral Galaxy Morphology
stronomers have long learned to classify spirals in terms of their morphological features, primarily their bulges, discs, and bars. In addition other properties...
Equinox, what a controversial concept! Since the dawn of archaeoastronomy this has arguably been the most problematic concept—perhaps together with the lunar...
Doing research is fighting, what any other thing the human being could do? Fight against powers or to get powers, that depends on us. Science can be a...
What is the Upper Limit on the Lightest Supersymmetric Higgs Mass?
In this talk the question of what is the upper bound on the lightest supersymmetric Higgs mass, m_h is addressed. This question is relevant since experimental...
What stars can tell us about galaxies: star formation histories in the Local Group
The formation and evolution of Local Group galaxies can be studied in the greatest possible detail thanks to the possibility of obtaining photometry and...