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Diffuse Gas and Cosmic Ecosystems SIG Seminar Series March 28, 2024

Time/Date: March 28, 2024 – 4pm ET / 1pm PT

Studying Cosmic Ecosystems with Holistic CGM Models

Speaker

Yakov Faerman, University of Washington

Abstract

The circumgalactic medium (CGM), through which gas flows into the galaxy from the cosmic web, and where energy and metals are deposited by galactic feedback, is an important component of cosmic ecosystems, shaping how galaxies evolve and affect the large-scale structure of the Universe. I will argue that flexible analytic models for the multiphase CGM are useful for fitting a wide range of multiwavelength observations and inferring the underlying gas properties, which can then be related to galaxy evolution, accretion and feedback processes, and gas small-scale physics. I will review recent results addressing the warm/hot phase of the CGM and describe ongoing work on the cool and intermediate-temperature phases, coupled with models for the virialized gas. I will then discuss how these combined, holistic models can help us prepare for the next generation of instruments and observatories, from small to large, including the Habitable Worlds Observatory.

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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.