We recently studied a small number of highly inclined spiral galaxies, and used their special geometry to determine absolute extinction values of the dust in...
Observations suggest that Asymptotic Giant Branch (AGB) stars contribute significantly to the dust budgets of galaxies, from our own Presolar Nebula to the...
Dust from AGBs: understanding the Spitzer observations of evolved stars in the Large Magellanic Cloud
Asymptotic Giant Branch (AGB) stars represent one of the main stellar sources for production of dust in the Universe. We provide a description of the formation...
Dust grain alignment in IC 63 - H2 formation enhancement and collisional disalignment
Interstellar dust grain alignment gives rise to polarization from UV to mm wavelengths, allowing the study of the geometry and strength of the magnetic field...
R Coronae Borealis stars (RCBs) provide an unique circumstellar environment that is hydrogen-deficient, helium-rich and carbon-rich in which dust condensation...
Dust in the Wind: testing a new paradigm for the nature of AGN feedback
Understanding the ouflows driven by Active Galactic Nuclei (AGN) is of key importance for the modern view of galaxy evolution. A recent paradigm shift in our...