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The centers of galaxies are complex environments whose properties are a result of the interactions between the massive black holes that reside there, vast clouds of gas, and dense populations of stars and stellar remnants.

Professor Rasio’s group studies numerical models of dense stellar environments such as nuclear star clusters.

Professor Larson’s group studies the interactions of single stars with massive black holes, a prospective LISA gravitational wave source class known as an EMRI (“extreme mass ratio inspiral”).

Professor Zadeh is an observer who studies stellar populations and physical processes in the Milky Way nucleus using observations across the electromagnetic spectrum.

Professor Fragione investigates the dynamical evolution of dense stellar environments including galactic nuclei. By using a combination of observational data, high precision simulation-based techniques, and analytical equations, he studies how the primordial properties of dense star clusters shape their fate and observable properties across cosmic time.

Galaxies are often attended by a group of dense stellar clusters orbiting in a vast area around the galaxy. These globular clusters are comprised of hundreds of thousands to millions of stars, and are held together by their mutual gravitational attraction.

Professor Rasio’s group uses numerical modeling techniques to simulate the evolution of globular clusters over the history fo the Universe, and studies how the observational properties of these clusters are derived from their evolutionary history.

Professors Kalogera and Larson collaborate closely with the globular cluster simulation group, since the clusters are potentially the home to large populations of gravitational wave sources observable by both LIGO and LISA.

Professor Geller uses both observations and simulations to study the dynamical evolution of open clusters, with a particular focus on the binary stars and exotic stars like blue stragglers and sub-subgiants.

Professor Muñoz studies the evolution of compact binaries in diverse environments such as globular clusters, with a focus on orbital resonances, dynamical friction and cluster tides.

Professor Fragione investigates the dynamical evolution of dense stellar environments including globular clusters. By using a combination of observational data, high precision simulation-based techniques, and analytical equations, he studies how the primordial properties of dense star clusters shape their fate and observable properties across cosmic time.

The close interaction of stars, stellar remnants, or combinations of both, will have dramatic consequences for the future evolution of the system and the long term properties of stellar populations. At CIERA these systems are studied both theoretically and observationally.

Professor Kalogera’s and Larson’s groups both use population synthesis to study expected rates and properties of merger events, which are strong gravitational wave sources for LIGO when they merge, and for LISA at earlier times during their inspiral.

Professors Fong is an observer who studies explosive transients that can result from stellar mass mergers, such as gamma ray bursts.

Professor Geller studies the products of collisions and mergers involving solar-type stars, which can result in blue stragglers, sub-subgiants and other exotic stars.

A star’s life cycle can be dramatically influenced by co-evolution with a binary companion. Repeated episodes of tidal interactions, mass transfer, or common envelope evolution will change the physical properties of the individual stars as well as the orbit they share.

Professors Kalogera and Larson both use population synthesis techniques to understand how binary interactions influence the properties observed across the entire population of binaries. They also explore how gravitational wave observations with LIGO and LISA can be used to elucidate the complex interaction history of binaries.

Professor Geller uses simulations and observations to study the products of binary mass transfer, often related to blue stragglers, sub-subgiants and other exotic stars.