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Astronomy Colloquium - JD Smith

Artist rendition of a Post-Starburst Galaxy, which are unlike other galaxies as they form as an aftermath of mergers/violent collisions between galaxies. Picture Credit: ALMA (ESO/NAOJ/NRAO)/S. Dagnello (NRAO/AUI/NSF)
September 29, 2022
3:00PM - 4:00PM
In Person & Online: Chem & Biomolecular Eng & Chem (CBEC) - Room 130; Zoom Webinar

Date Range
Add to Calendar 2022-09-29 15:00:00 2022-09-29 16:00:00 Astronomy Colloquium - JD Smith Title: After the Fall: The Dust and Gas in Post-Starburst Galaxies Abstract: A class of rare, rapidly quenched galaxies called Post-Starbursts (PSB) has played a unique role in galaxy evolution frameworks.  Originally thought to be the simple stellar-dominated young analogs of quiescent systems, our understanding has shifted radically over the past decade and a half.  PSBs have serendipitously been found to harbor unexpectedly large reservoirs of gas and dust in compact, turbulent cores, rivaling gas densities found in ULIRGs, but with star formation efficiencies suppressed by factors of ten.  I'll describe the historical and very recent progress in cracking the code of the unusual ISM properties of these enigmatic systems. Speaker: JD Smith (University of Toledo) Artist rendition of a Post-Starburst Galaxy, which are unlike other galaxies as they form as an aftermath of mergers/violent collisions between galaxies. Picture Credit: ALMA (ESO/NAOJ/NRAO)/S. Dagnello (NRAO/AUI/NSF) In Person & Online: Chem & Biomolecular Eng & Chem (CBEC) - Room 130; Zoom Webinar Department of Astronomy astronomy@osu.edu America/New_York public

Title: After the Fall: The Dust and Gas in Post-Starburst Galaxies

Abstract:

A class of rare, rapidly quenched galaxies called Post-Starbursts (PSB) has played a unique role in galaxy evolution frameworks.  Originally thought to be the simple stellar-dominated young analogs of quiescent systems, our understanding has shifted radically over the past decade and a half.  PSBs have serendipitously been found to harbor unexpectedly large reservoirs of gas and dust in compact, turbulent cores, rivaling gas densities found in ULIRGs, but with star formation efficiencies suppressed by factors of ten.  I'll describe the historical and very recent progress in cracking the code of the unusual ISM properties of these enigmatic systems.

Speaker: JD Smith (University of Toledo)

Artist rendition of a Post-Starburst Galaxy, which are unlike other galaxies as they form as an aftermath of mergers/violent collisions between galaxies. Picture Credit: ALMA (ESO/NAOJ/NRAO)/S. Dagnello (NRAO/AUI/NSF)

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