Astrophysics Seminars

Apr
19
2011

Institute for Advanced Study Astrophysics Seminar

Diverse Energy Sources for Supernovae
Lars Bildsten
11:00am|Bloomberg Hall Astrophysics Library
ABSTRACT: The theoretical community is beginning to appreciate (and predict) the potential diversity of explosive outcomes from stellar evolution while the supernovae surveys are finding new kinds of supernovae. I will speak about two such new...
Apr
14
2011

Institute for Advanced Study Informal Astrophysics Seminar - TITLE ADDED

Dark Energy Measurements from Supernovae: One Observationalist's Mid-Semester Report Card
11:30am|Bloomberg Hall Astrophysics Library
ABSTRACT: A decade since the realization that our universe's expansion is accelerating, the ball remains in the observationalists' court -- as the theorists look for more constraints on the parameter space.I will discuss some of the progress that...
Apr
05
2011

Institute for Advanced Study Astrophysics Seminar

Galaxy Gas Flows
Mary Putman
11:00am|Bloomberg Hall Astrophysics Library
ABSTRACT: Many galaxies exhibit the need for a continual source of star formation fuel. Halo gas is a common feature of these galaxies, though utilizing this gas as fuel may require the gas to go through multiple phases. I will discuss new...
Mar
31
2011

Institute for Advanced Study Informal Astrophysics Seminar

Gravitational Wave Astronomy in the Advanced Detector Era
Sean T. McWilliams
11:30am|Bloomberg Hall Astrophysics Library
ABSTRACT: With the imminent start of Advanced LIGO/VIRGO observations, and the less imminent but much hoped-for advent of LISA, gravitational wave science will transition from a specialty of theoretical astrophysics and experimental interferometry...
Mar
24
2011

Institute for Advanced Study Informal Astrophysics Seminar

Super-Eddington Accretion Disks
11:30am|Bloomberg Hall Astrophysics Library
ABSTRACT: I will review our present understanding of super-Eddington atmospheres, as borne from theory and observations. In particular, I will show how atmospheres can sustain super-Eddington fluxes, while accelerating only ``moderate'' mass loss...