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Astronomy Seminar

Friday, January 24, 2025 11:00 AM – 12:00 PM
  • Location
    Gant South Building
  • Description
    Dr. Jakob den Brok, Center for Astrophysics | Harvard & SmithsonianUnveiling Molecular Gas Conditions and their link to Star Formation with CO Observations in Nearby Galaxies An intricate interplay exists between the molecular gas in the interstellar medium (ISM) and the onset of star formation. Gaining insight into the molecular gas's composition and its physical and chemical conditions is crucial to comprehending how star formation is regulated, and how galaxies evolve. However, the most abundant molecule, H_2, is challenging to observe directly under commonly cold ISM conditions across nearby galaxies. Carbon Monoxide (CO) emission has become the most accessible tracer of the bulk molecular ISM distribution. I will present recent findings from multiple comprehensive astrophysical surveys mapping CO and isotopologue line emission across entire nearby galaxies. With these, I explore the CO excitation conditions from kiloparsec to 100s-parsec scales and show how it is possible to also assess the chemical enrichment of C and O elements. Furthermore, I present the analysis of variations in the CO-to-H_2 conversion factor, which is needed accurately translate the observed CO brightness into a H_2 mass surface density. I link these variations to different galactic environments across the entire molecular disk of iconic star-forming galaxies such as M51 and M101. In summary, my talk illustrates the use of CO line observations as diagnostics for accurately accounting and interpreting the variation of CO-derived properties of the molecular ISM from kiloparsec to 100s-parsec scales.
  • Website
    https://events.uconn.edu/physics-department/event/715475-astronomy-seminar

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