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Diffuse Gas in Cosmic Ecosystems SIG Seminar Sept 26, 2024

September 26, 2024 – 4pm ET / 1pm

New Constraints on Thermodynamic Profiles of the Outer Circumgalactic Medium

Speaker

Nicholas Battaglia, Cornell University

Abstract

An exciting new window into the circumgalactic medium (CGM) has opened up with the recent observations of the thermal and kinetic Sunyaev-Zel’dovich (SZ) effects on galactic spatial scales. After introducing the SZ effects, I will present the ongoing efforts to extract these galaxy scales SZ signals in data from the Atacama Cosmology Telescope. I will show how these observations are currently being used to constrain important physical processes, like feedback, that govern galaxy formation. Additionally, I will present the puzzle these observations pose to state-of-the-art cosmological simulations. I will conclude by highlighting the expected rapid growth in such SZ observations over the next decade with the upcoming millimeter and sub-millimeter focused experiments, like the Simons Observatory, CCAT, and CMB-S4.

Zoom link

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.