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Full-Text Articles in Physical Sciences and Mathematics
Using Nasa's Tess Mission To Search For Extremely Low Mass White Dwarf Stars, Corinna Peña
Using Nasa's Tess Mission To Search For Extremely Low Mass White Dwarf Stars, Corinna Peña
Undergraduate Honors Thesis Collection
Extremely low-mass white dwarf stars (ELM) are white dwarf stars with a mass lower than 0.45 solar masses that could not have evolved through normal processes within the lifetime of our universe. Therefore, these objects can only be created through a common envelope phase or a stable Roche lobe overflow while in a binary. These objects have periods between a few minutes to a few hours, so they are very short lived which makes them very rare. My goal for this project was to find these ELM stars by using NASA's Transiting Exoplanet Survey Satellite (TESS) data. I analyzed this …
The Role Of Black Hole And Neutron Star Interaction On The Dynamical Evolution Of Dense Stellar Systems, Michael Pajkos
The Role Of Black Hole And Neutron Star Interaction On The Dynamical Evolution Of Dense Stellar Systems, Michael Pajkos
Undergraduate Honors Thesis Collection
With the recent detection of gravitational waves from the Laser Interferometer Gravitational-Wave Observatory, or LIGO, a new realm of gravitational astrophysics has been opened. As the process of observing gravitational wave signals is still in its infancy, there is a need to provide gravitational astronomers with observable signatures in the electromagnetic spectrum. Hence, we explore the impact of solar mass black holes on the morphology of globular clusters. It has long been thought that due to high kick velocities from compact object gravitational interaction, Galactic age Globular Clusters are unable to retain black holes. Recent simulations, however, suggest that a …
Constraining The Parameters Of Six Known Transiting Exoplanets, Mackenzie Lee Jones
Constraining The Parameters Of Six Known Transiting Exoplanets, Mackenzie Lee Jones
Undergraduate Honors Thesis Collection
We present two new transits of GJ~1214b, five of TrES-lb, two of XO~2b, and one each of TrES~3b)WASP-16b and WASP- 36b. These observations were made with multiple observatories including IRTF-MORIS, Butler University's Holcomb Observatory, SARA-KPNO, and SARA-eTIO. Due to poor conditions and a lack of good comparison stars within the field of view, the parameter values for the radius ratio, inclination, and orbital distance, found for GJ-1214b are not reliable. The timing values, while still suspect, suggest consistency with the current ephemeris. After further analysis, the radius ratio we found for TrES-1b in Sloan r' is 0.0.13501±0.0001l, which differs by …
The Effect Of Tidal Disruptions On Giant Stars In The Galactic Center, Brian B. Geiss
The Effect Of Tidal Disruptions On Giant Stars In The Galactic Center, Brian B. Geiss
Undergraduate Honors Thesis Collection
Recent observational data suggest the depletion of late-type giant stars in the inner most region of the Galactive Nucleus. Using dynamically evolving Fokker-Planck models of the Galactic Nucleus, we have followed in detail the stellar distribution as it evolves through the postmain-sequence phases. Of particular interest was the effect of stellar collisions and tidal disruptions by the central massive black hole on post main sequence stars as they expand in size. B y modeling tidal disruptions and stellar collisions, we have found that there should be a significant depletion of the giant stars in the innermost regions of the nucleus. …