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Skip to Search Results- 2Avendano Nandez, Jose L
- 2Van, Kenny
- 1Deb, Soumen
- 1Gazer, Reuben S.
- 1Gladstone, Jeanette
- 1Hamilton, Michée-Ana
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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...
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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...
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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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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 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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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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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 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...