DARKNESS VISIBLE: Dark Matter in astrophysics and particle physics
2 August 2010 - 6 August 2010
The Institute of Astronomy, Cambridge, summer conference will focus on Dark Matter, bring together recent progress in astrophysical studies, direct and indirect detection experiemnts, and the LHC.
We invite applications for contributed talks and posters to fill an expanded format for the Darkness Visible meeting to be held at the Institute of Astronomy, Cambridge (UK). This meeting will bring together particle- and astro - physicists (theoretical, experimental and observational) to present recent advances in our understanding of dark matter at scales ranging from particle pysics to cosmology.
Angular Momentum Transport and Energy Release in Accretion Discs
7 September 2009 - 8 September 2009
The aim of this conference is to bring together an outstanding group of young researchers to discuss theoretical and observational progress toward understanding accretion disc physics in Young Stellar Objects, compact binaries, and galactic nuclei.
Putting Gravity to Work
21 July 2008 - 25 July 2008
Putting Gravity to Work: from black holes to galaxy clusters was a high energy astrophysics conference held at the Institute of Astronomy, Cambridge, in celebration of Andy Fabian's 60th birthday.
The Planet-Disc Connection
17 July 2006 - 21 July 2006
Observations of the later evolutionary stages of discs around young stars offer the best opportunity to study planet formation from an observational perspective. Localised clearing of dust and gas in discs can be inferred from a variety of imaging/spectroscopic diagnostics and is often interpreted as evidence for planet formation; alternatively, such clearing results from some other process which needs to be taken into account when assessing the environment in which planets form.
Starbursts - From 30 Doradus to Lyman break galaxies
6 September 2004 - 10 September 2004
Large-scale starbursts are very common features of early galaxy evolution. At high redshifts, the majority of the present-day "normal" galaxy progenitors either appear to be undergoing violent gravitational interactions, or experience very active star formation throughout.
