Astrophysics Seminars

Jan
19
2010

Institute for Advanced Study Informal Astrophysics Seminar - DIFFERENT DAY

Planetary Systems, Turbulence and Saturn's Rings
11:30am|Bloomberg Hall Astrophysics Library
The discovery of more than 400 extrasolar planets keeps challenging the theory of planet formation. Multi-planetary systems are of particular interest. Their orbital parameters allow us to constrain properties of the otherwise unobservable formation...
Jan
12
2010

Institute for Advanced Study Informal Astrophysics Seminar - DIFFERENT DAY

Testing AGN Evolution Models Through the Comparison of Semi-Analytic Simulations and a Large Observational Data Set
Amy Kimball
11:30am|Bloomberg Hall Astrophysics Library
Quasars and radio galaxies display great morphological variety that correlates with other properties such as spectral slope and luminosity. The unification theory for radio-loud active galactic nuclei (AGNs) attempts to explain much of this...
Dec
10
2009

Institute for Advanced Study Informal Astrophysics Seminar

Cosmology and Astrophysics with Galaxy Clusters
Daisuke Nagai
11:30am|Bloomberg Hall Astrophysics Library
Clusters of galaxies are unique and powerful probes of cosmology and astrophysics, promising to provide new insights into the nature of dark energy and dark matter to the physics of galaxy formation. The study of galaxy clusters combines the...
Dec
03
2009

Institute for Advanced Study Informal Astrophysics Seminar

Satellite Galaxies in LCDM: Orbits, Merging & Disruption
Andrew Wetzel
11:30am|Bloomberg Hall Astrophysics Library
Dark matter halos that merge with larger halos persist as subhalos, which host satellite galaxies. While subhalos are rapidly stripped of their dark mass, the compact luminous material remains intact for some time. I use a high-resolution...
Nov
19
2009

Institute for Advanced Study Informal Astrophysics Seminar

The Effective Theory of Quintessence and Its Observational Signatures
Guido D'Amico
11:30am|Bloomberg Hall Astrophysics Library
I will study generic single-field dark energy models, by a parametrization of the most general theory of their perturbations around a given background, including higher derivative terms. In appropriate limits this approach reproduces standard...