DGCE SIG Seminar
Diffuse Gas in Cosmic Ecosystems Science Interest Group
DATE
July 24, 2025
TIME
4:00 pm EST
COMMUNITY
DGCE SIG
TYPE
Seminar
Uncovering Hidden Astrophysical Laboratories with (Diffuse) Molecular Hydrogen
Keri Hoadley, University of Florida
Molecular hydrogen (H2) permeates almost all regions of cool cosmic ecosystems- from the molecular clouds that stars form in, to planet-forming gaseous disks, and the space between stars in galaxies. It is, however, notoriously hard to detect, given the quantum properties of the molecule, and we often rely on other proxies to infer what H2 in present in many systems. Where we have observed diffuse H2, particularly fluorescing H2, has revealed some extraordinary astrophysical laboratories we may have missed otherwise. In this talk, I will bring to light a few ways we have observed fluorescing H2 that have revealed unique systems that warrant further study in the evolution of cosmic ecosystems and stars: the Blue Ring Nebula, and the Eos cloud. Time permitted, I’ll discuss a few ways we can continue to use fluorescing H2 to further advance our knowledge of cosmic ecosystem evolution, using planned/upcoming UV missions, UV mission concepts, and UV capabilities on HWO.
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