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Colloquium – Chris Hayward’s “Bursty star formation: physical drivers and implications for JWST observations of high-redshift galaxies”
October 26, 2023 @ 12:45 pm - 1:45 pm
“Bursty star formation: physical drivers and implications for JWST observations of high-redshift galaxies”
Abstract:
A complete theory of galaxy formation requires understanding the details of how gas is converted into stars over cosmic time, which is affected by gas supply, star formation, and feedback-driven outflows. Based on the results of state-of-the-art cosmological zoom simulations, I will argue that galaxy formation is a violent process: at high redshift, stellar feedback causes all star-forming galaxies to undergo rapid fluctuations in their star formation rates on ~10-Myr timescales. Bursts of star formation are followed by strong outflows, which cause the star formation rate to drop precipitously. Fresh gas supply from galactic fountains rejuvenates star formation and restarts the cycle. At z ~ 1, simulations of massive galaxies exhibit a qualitative transition: outflows are no longer driven effectively, and the galaxies transition to steadily star-forming, well-order disk galaxies. I will discuss the physical causes of bursty star formation and the aforementioned transition to time-steady star formation, in addition to some implications for JWST observations of high-redshift galaxies.
Chris Hayward, Center for Computational Astrophysics
Thursday, October 26, 2023 @ 12:45 PM – 1:45 PM EST
217 Bryant Space Science Center