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Skip to Search Results- 2Avendano Nandez, Jose L
- 2Van, Kenny
- 1Bridges, Jake E.
- 1Deb, Soumen
- 1Gazer, Reuben S.
- 1Hughes, Andrew
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Fall 2013
The equation of state for cold ultra-dense matter has puzzled astrophysicists for decades. This is because the conditions of supra-nuclear density matter, such as those in neutron stars, are not terrestrially replicable. X-ray light curves from accreting neutron stars have proven to be useful...
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Spring 2021
Relativistic jets are an ubiquitous element of systems with accreting black holes. These jets carry away a large fraction of the accreted energy which later energizes their surrounding media. On the largest scales, the jets from supermassive black holes found in the center of galaxies provide a...
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Fall 2022
In astrophysics, stellar evolution is one of the most discussed topics. Although a significant amount of research and advancement of instrumentation over the last few decades have contributed to this field greatly, our understanding of the pre-main sequence evolution remains largely incomplete....
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Fall 2017
In this thesis we investigate a novel binary formation channel with a semi- degenerate donor and examine the stability criteria in binary systems with a massive donor. First we will review the current basics in the understanding of binary systems along with where recent research has been moving...
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Spring 2018
We explore the production and observation of high energy (X-ray and ultraviolet/UV) radiation in the context of Galactic, compact binary systems. At the end of the stellar lifecycle, a star collapses into one of three compact objects (COs) depending on the mass at the time of collapse: a white...
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Fall 2021
In this thesis, we investigate the effectiveness of theoretical descriptions of angular momentum loss in stars due to the presence of magnetic fields, a process commonly known as magnetic braking. The most widely used description of magnetic braking is the so-called Skumanich prescription, which...
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Connecting galactic to local scales in the neutral interstellar medium across the Local Group
DownloadFall 2020
Star formation drives secular galaxy evolution by linking stars and gas in galaxies. This link forms part of the "baryonic cycle," where stars form from interstellar gas, and a portion of that gas is returned to the interstellar medium upon the star’s death. Understanding the baryonic cycle and...
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Fall 2015
Interactions between stars are crucial for diverse areas of astrophysics, but they are not yet fully understood. These interactions come in forms as diverse as a direct physical collision, matter transfer from one star to another, and a "common envelope" (CE). The CE phase is a short period of...