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- <b>ASTRONOMY COLLOQUIUM</b><br>Tracing the Cosmic Shutdown of Star Formation in Massive Galaxies
- <b>ASTRONOMY COLLOQUIUM</b><br>The Effects of Magnetic Field Morphology on the Determination of Oxygen and Iron Abundances in the Solar Photosphere
- <b>ASTRONOMY COLLOQUIUM</b><br>Star Formation Across Space
- <b>ASTRONOMY COLLOQUIUM</b><br>Lonely Galaxies: The Baryon Content of Isolated Dwarf Galaxies
- <b>ASTRONOMY COLLOQUIUM</b><br>Choose Your Own Adventure: Multiplicity of Planets Among the Smallest Stars
- <b>ASTRONOMY COLLOQUIUM</b><br>Why the Invisible Reservoir of Gas Around Galaxies Counts in Galaxy Evolution
- <b>ASTRONOMY COLLOQUIUM</b><br>A Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole
- ASTRONOMY COLLOQUIUM
- ASTRONOMY COLLOQUIUM<br>Better Living Through Computation: Exploring the First Generations of Galaxies with Large-Scale Simulations
- ASTRONOMY COLLOQUIUM<br>The Search for Earth 2.0
- ASTRONOMY COLLOQUIUM<br>The Fast and Furious Lives of High Velocity Clouds
- ASTRONOMY COLLOQUIUM<br>Supernovae as Drivers of Dust Evolution in Galaxies
- ASTRONOMY COLLOQUIUM<br>How to Measure the Composition of Planet-Forming Material
- ASTRONOMY COLLOQUIUM<br>Direct Imaging of Extrasolar Planets and the Gemini Planet Imager
- ASTRONOMY COLLOQUIUM<br>Blowing in the Quasar Wind: Feedback from Black Hole Outflows in Major Galaxy Mergers
- ASTRONOMY COLLOQUIUM<br>Magellan/MDM Colloquium: Department Members Share Their Current Work Using Magellan/MDM Observatories
- ASTRONOMY COLLOQUIUM<br>The Fisk-Vanderbilt Masters-to-PhD Bridge Program: A Model for Increasing Diversity at the PhD Level in Physics & Astronomy
- ASTRONOMY COLLOQUIUM<br>Science, Symphony, and the Northern Lights
- ASTRONOMY COLLOQUIUM<br>Observing the Formation of Planetary Diversity
- ASTRONOMY COLLOQUIUM<br>Lies, Damned Lies, and Statistics: Empirical Constraints on Theories of Planet Formation
- ASTRONOMY COLLOQUIUM<br>Black People in Astronomy: Why So Few?
- ASTRONOMY COLLOQUIUM <br> Hot on the Trail of Warm Planets Orbiting Cool Stars
- ASTRONOMY COLLOQUIUM<br>Galaxy Clusters as Cosmological and Astrophysical Probes
- ASTRONOMY COLLOQUIUM <br> Discovery of a Thorne-Zytkow Object Candidate in The Small Magellanic Cloud
- ASTRONOMY COLLOQUIUM<br>Where's the Matter? (Tales from the Milky Way's Destructive Past)
- ASTRONOMY COLLOQUIUM<br>Measuring the Mass-Radius Relation of Neutron Stars
- ASTRONOMY COLLOQUIUM <br> Accretion Disk Outbursts: MHD Simulations (Finally) Confront Reality
- ASTRONOMY COLLOQUIUM <br> The Observability of Recoiling Black Holes as Offset Quasars
- ASTRONOMY COLLOQUIUM<br>Black Hole Masses in Active Galaxies
- ASTRONOMY COLLOQUIUM<br>Using Multiwavelength Variability Studies to Probe the Disk-Jet Connection of Fermi Blazars
- ASTRONOMY COLLOQUIUM<br>X-ray Reverberation Mapping in AGN
- 3rd Annual Astronomy Undergraduate Poster Session
- ASTRONOMY COLLOQUIUM<br>High-Energy-Density Astrophysics in the Laboratory
- SPECIAL ASTRONOMY COLLOQUIUM<br>Ralph Baldwin Prize in Astrophysics and Space Sciences<br>Lonely Massive Stars</br>
- ASTRONOMY COLLOQUIUM<br>Live Fast Die Young: The Evolution of Massive Stars towards their Death</br>
- ASTRONOMY COLLOQUIUM<br>Watching a Little Gas Cloud on its Way into the Galactic Supermassive Black Hole
- ASTRONOMY COLLOQUIUM<br>Dwarf Galaxies as Cosmological Probes
- SPECIAL ASTRONOMY COLLOQUIUM<br>The Magellan and MDM Observatories / Michigan Astronomy
- ASTRONOMY COLLOQUIUM<br>Seeing Worlds in Grains of Sand
- ASTRONOMY COLLOQUIUM<br>Mohler Prize Lecture<br>Lighting up the Universe: Witnessing Cosmic Dawn</br>
- ASTRONOMY COLLOQUIUM<br>The ALFALFA Census of Gas-Bearing Galaxies at z=0</br>
- ASTRONOMY COLLOQUIUM<br>Accretion Disk Outbursts: MHD Simulations (Finally) Confront Reality
- ASTRONOMY COLLOQUIUM<br>3D Spectroscopy of Giant H II Regions in Nearby Spiral Galaxies</br>
- ASTRONOMY COLLOQUIUM<br>Star Clusters and High Mass X-Ray Binaries in Nearby Spirals, Mergers, and Starburst Galaxies
- PUBLIC ASTRONOMY DISTINGUISHED ALUMNUS COLLOQUIUM | Cracking the Cosmic Code
- ASTRONOMY DISTINGUISHED ALUMNUS COLLOQUIUM
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Fundamental questions remain unanswered in understanding galactic-scale star formation, despite many decades of investigation and progress. These include: how do stars cluster in galaxies, and how do these structures evolve in time? Do we actually have "clustered" and "diffused" modes of star formation? When structures remain bound (star clusters), how do their populations evolve? How are they related to the galactic-scale star formation? Is the stellar Initial Mass Function universal? How are popular star formation rate indicators affected by the recent star formation history of a galaxy? How are these effects impacting our understanding of the scaling laws of star formation with the gas reservoir? The answers to these questions inform our theories for the evolution of galaxies through cosmic times. Many of these questions are being addressed by recent projects that combine UV and high-angular resolution with the Hubble Space Telescope, and which I will describe together with the results they have obtained so far.
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