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dc.contributor.advisorRulis, Paul Michael, 1976-
dc.contributor.advisorUkpokodu, Omiunota Nelly
dc.contributor.authorWeston, Madalyn Elizabeth
dc.date.issued2022
dc.date.submitted2022 Spring
dc.descriptionTitle from PDF of the title page viewed June 27, 2022
dc.descriptionDissertation advisors: Paul Rulis and Omiunota Ukpokodu
dc.descriptionVita
dc.descriptionIncludes bibliographical references (pages 110-137)
dc.descriptionThesis (Ph.D.)--Department of Physics and Astronomy; School of Education. University of Missouri--Kansas City, 2022
dc.description.abstractSimulations of gas-rich, major galaxy mergers predict elevated amounts of star formation (SF) and nuclear black hole growth (active galactic nuclei, or AGN). This model is supported by observations that find enhanced SF in mergers, but support for the AGN-merger connection remains uncertain. Interstellar dust, a bi-product of SF, can block much of the light from an AGN and re-radiate that energy at infrared (IR) wavelengths. Therefore, quantifying the amount of buried AGN activity in the IR is key to understanding the role of major mergers in galaxy evolution. Spectral energy distributions (SEDs) allow Astrophysicists to disentangle AGN activity from SF. I hypothesize that applying SED analysis to a sample of merging galaxies will show an enhancement in AGN activity over control galaxies. I perform SED analysis from the far-ultraviolet (FUV) to the mid-IR on a sample of 49 merging galaxies and 49 statistically-matched control galaxies in the nearby universe. I find that the SED AGN luminosity correlates with the [OIII] luminosity, a common indicator of AGN power. I find that galaxies previously identified as Seyfert or WISE AGNs generally have a higher SED AGN luminosity. I do not find an increased occurrence of SED-detected AGNs in merging over control galaxies, rejecting our study hypothesis. To meet the interdisciplinary requirements of this degree, I also design a new graduate-level course in Multicultural Education for STEM (science, technology, engineering and mathematics) fields. “Diversity and Inclusion” have become buzz words in STEM, as research continues to show achievement and participation gaps for women, people of color, disabled persons, those of low socio-economic status, and members of the LGBTQIA+ community. Research about the STEM gaps has existed for decades, particularly with respect to teaching practices that contribute to under-representation. Yet little change has occurred in STEM classrooms. Graduate students (i.e., future STEM professors and industry leaders) stand in a unique position to impact diversity and inclusion efforts. Through targeted education centered on diversity and inclusion in teaching methods, we can produce a new generation of STEM educators who are aware and mindful of their unique role in fighting inequality in STEM.
dc.description.tableofcontentsIntroduction -- Sample selection -- Analysis -- Discussion -- Summary -- Multicultural education in STEM fields: A new course for STEM majors at the graduate level
dc.format.extentxii, 138 pages
dc.identifier.urihttps://hdl.handle.net/10355/90576
dc.subject.lcshGalaxy mergers
dc.subject.lcshSpectral energy distribution
dc.subject.lcshScience -- Study and teaching
dc.subject.otherDissertation -- University of Missouri--Kansas City -- Physics
dc.subject.otherDissertation -- University of Missouri--Kansas City -- Education
dc.titleFar-UV to Mid-IR Spectral Energy Distributions of Nearby Merging Galaxies
thesis.degree.disciplinePhysics (UMKC)
thesis.degree.disciplineCurriculum and Instruction (UMKC)
thesis.degree.grantorUniversity of Missouri--Kansas City
thesis.degree.levelDoctoral
thesis.degree.namePh.D. (Doctor of Philosophy)


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