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UR: Modeling Chemical Abundance Evolution in Dwarf Galaxies

UR: Modeling Chemical Abundance Evolution in Dwarf Galaxies

by Guest | Mar 28, 2021 | Undergraduate Research

In the latest of our #UndergradResearch series, discover how Alexandra Kwon modeled the evolution of chemical abundance in dwarf galaxies.

UR: Understanding the Balance of Star Formation and Black Holes in Nearby Luminous Infrared Galaxies

UR: Understanding the Balance of Star Formation and Black Holes in Nearby Luminous Infrared Galaxies

by Guest | Mar 21, 2021 | Undergraduate Research

In today’s #UndergradResearch post, Meredith Stone shares how she used Spitzer spectra to learn about the evolution of galaxies through their star formation and AGN activity.

UR: The Orbit and Growth of HD 142527B

UR: The Orbit and Growth of HD 142527B

by Guest | Mar 14, 2021 | Undergraduate Research

In the latest of our #UndergradResearch series, discover William Balmer’s research on how direct imaging can show us more about planet formation!

UR: I Spy Transits and Pulsations – Empirical Variability in White Dwarfs Using Gaia and the Zwicky Transient Facility

UR: I Spy Transits and Pulsations – Empirical Variability in White Dwarfs Using Gaia and the Zwicky Transient Facility

by Guest | Mar 7, 2021 | Undergraduate Research

Today’s #UndergradResearch post by Joseph Guidry is all about searching for variable white dwarf stars!

UR: An Alert-Broker for Real-Time Astronomical Events

UR: An Alert-Broker for Real-Time Astronomical Events

by Guest | Mar 5, 2021 | Undergraduate Research

In the latest of our #UndergradResearch series, discover how Sarah DeSantis automatically identified which stars of the many observed were behaving strangely and what these objects may be.

UR: Investigating Spatially Resolved Gas Flows Around the Milky Way

UR: Investigating Spatially Resolved Gas Flows Around the Milky Way

by Guest | Mar 2, 2021 | Undergraduate Research

In our latest of our undergrad research series, discover how the Milky Way’s gas flow can be measured and how this can determine the Milky Way’s future.

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