OASIS high-resolution integral field spectroscopy of the SAURON ellipticals and lenticulars
We present a summary of high-spatial resolution follow-up observations of the elliptical (E) and lenticular (S0) galaxies in the SAURON survey using the OASIS...
Stellar rotation, parameterized by a star's projected rotational velocity v sin i, is a fundamental parameter linked to star formation, evolution, and dynamical...
From observations taken with the Wide Field Camera (WFC) at the Isaac Newton Telescope (INT), we have built an astrometric and photometric catalogue of stars in...
We studied the nuclear obscuration of galaxies hosting Low Ionization Narrow Emission Regions (LINERs) based on their X-ray and optical emission. X-ray data...
Obscured stellar clusters and nuclear activity in seyfert galaxies
Starbursts and AGNs are frequently coupled in the central kiloparsecs of seyfert galaxies, where molecular gas plays a critical role in fueling nuclear...
Observability and Geometry in Three Dimensional Quantum Gravity
We consider the coupling between massive and spinning particles and three dimensional gravity. This allows us to construct geometric operators (distances...
We study a family of physical observable quantities in quantum gravity. We denote them W functions, or n-net functions. They represent transition amplitudes...