BEGIN:VCALENDAR
VERSION:2.0
X-WR-CALNAME;VALUE=TEXT:Seminar - Natalie Nicole Sanchez (U Washington)
PRODID:-//Harvard events data//EN
BEGIN:VEVENT
UID:event_1414895_0
SUMMARY:Seminar - Natalie Nicole Sanchez (U Washington)
DESCRIPTION:<p>	<style type="text/css"><!--td {border: 1px solid #ccc;}br {mso-data-placement:same-cell;}-->	</style>	Connecting Cosmic Gas Flows and Metal Enrichment to Supermassive Black Hole Growth in Galactic Evolution"</p><p>	<style type="text/css"><!--td {border: 1px solid #ccc;}br {mso-data-placement:same-cell;}-->	</style>	In this talk, I will discuss the impact of supermassive black hole (SMBH) feedback on the gas phase evolution of Milky Way-mass (MW-mass) galaxies. Both my simulation suites were created with the N-body+Smoothed particle hydrodynamics code, ChaNGa, and include a 25 Mpc cosmological volume, Romulus25, and a suite of "genetically modified" (GM) galaxies. These GM galaxies originate from nearly identical initial conditions resulting in minor modifications to their accretion histories that maintain the large scale structure and final main halo mass of the original simulation. Exploring the MW-mass galaxies from these combined simulation suites, we find that (1) the SMBH propagates metals from the disk out into CGM, (2) how much metal is retained in the ISM (and CGM) depends on the SMBH's deviation from the M-sigma relation, and (3) black hole accretion histories can be influenced by larger-scale galaxy accretion physics, which work in tandem to quench star formation.</p><p>	 </p>
LOCATION:Zoom
STATUS:CONFIRMED
DTSTART:20210927T153000Z
DTEND:20210927T160000Z
END:VEVENT
END:VCALENDAR