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dc.contributor.advisorRangelov, Blagoy
dc.contributor.authorLuitel, Sudarshan ( )
dc.date.accessioned2021-07-22T16:46:08Z
dc.date.available2021-07-22T16:46:08Z
dc.date.issued2021-08
dc.identifier.citationLuitel, S. (2021). Numerical simulation of high velocity stars (Unpublished thesis). Texas State University, San Marcos, Texas.
dc.identifier.urihttps://digital.library.txstate.edu/handle/10877/14053
dc.description.abstractThe origins of high velocity runaway stars have been of interest since their discovery. To shed some light on this important problem in modern astrophysics, we use rapid binary stellar evolution code. We have simulated hundreds of thousands of massive stars in binaries and track their dynamical evolution. We discuss our findings in this work. We show the results for runaway compact objects and regular stars, and discuss the implications of our results. When available, we compare our simulations with observational data.
dc.formatText
dc.format.extent51 pages
dc.format.medium1 file (.pdf)
dc.language.isoen
dc.subjectSimulation
dc.subjectNeutron star
dc.subjectBlack hole
dc.titleNumerical Simulation of High Velocity Stars
txstate.documenttypeThesis
dc.contributor.committeeMemberOlson, Donald
dc.contributor.committeeMemberBanzatti, Andrea
thesis.degree.departmentPhysics
thesis.degree.disciplinePhysics
thesis.degree.grantorTexas State University
thesis.degree.levelMasters
thesis.degree.nameMaster of Science
dc.description.departmentPhysics


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