Date of Graduation

5-2022

Document Type

Thesis

Degree Name

Bachelor of Science

Degree Level

Undergraduate

Department

Physics

Advisor/Mentor

Lehmer, Bret

Committee Member/Reader

Kennefick, Daniel

Committee Member/Second Reader

Ward, Barry

Committee Member/Third Reader

Morrissey, Sean

Abstract

We construct reasonably accurate models of the X-Ray spectra of a multitude of sources in M51. We construct both average and individual models for the sources, which are split into 16 groups as the counts per source increases. Then, we create a plot to show how the model-predicted values of column density (nH) and photon index (gamma) change with luminosity. These models will be used to create an accurate X-Ray stellar energy distribution (SED) for M51, and to better understand how the SED changes with environmental factors like metallicity and star formation rate (SFR).

Keywords

X-ray, luminosity, star formations, metallicity

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