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PUG Seminar

PUG Seminar

Whitmore 321

2025-11-07

Abstract: Be/X-ray Binaries (BeXRB) are a common type of X-ray binary star system taht emit variable radiation across the electromagentic spectrum on all timescales. In this talk, I will discuss the different observational properties of BeXRBs and describe the underlying physical process at work. Through these processes, we will gain a better understanding of how BeXRBs can improve our understanding of the evolution of high-mass stars and compact objects.

Schedule for PUG Seminar
TimeSpeakerTitle
11:00Thomas GaudinAn Overview of Broadband Emission in Be/X-ray Binary Systems

About our wordmark
Monica The IGC wordmark was created by Monica Rincon Ramirez, while she was a graduate student at the Institute for Gravitation and the Cosmos (IGC). Monica enjoys drawing new connections between fundamental theory and observations. Her graduate work includes specialized topics in general relativity, loop quantum gravity, and quantum fields in cosmological backgrounds. In particular, her thesis work focused on finding effective quantum corrections to gravitational phenomena from spinfoams, and applications to cosmology. She received her PhD in 2024.

The wordmark symbolizes the scope and variety of research at the IGC. The base of the image represents quantum gravity, evoking the quantum geometrical picture from spinfoams and loop quantum gravity. These are among the approaches to fundamental questions studied at the Center for Fundamental Theory. The middle of the image represents the Center for Theoretical and Observational Cosmology by galaxies embedded in a smooth surface, characteristic of spacetime in general relativity and the much larger physical scales studied in cosmology. Finally, at the top, the surface curves to an extreme, representing a supermassive black hole accompanied by an energetic jet. These elements depict an active galactic nucleus, inspired by Centaurus A. Just to the right, a pair of black holes approaches merger. This top portion of the wordmark represents the Center for Multimessenger Astrophysics, which specializes in the study of high-energy phenomena in the universe.