Probing the Multiplicity of Dusty Wolf-Rayet Stars with Multi-Wavelength Techniques: Survey of Infrared Spectrometry
Faculty Mentor Name
Noel Richardson
Format Preference
Poster
Abstract
Wolf-Rayet (WR) stars, emblematic of massive celestial entities in advanced evolutionary phases, wield significant influence over the cosmic background. Carbon-rich WR stars emerge prominently among their ranks, distinguished by their expansive infrared emissions, which foster unique conditions conducive to producing cosmic dust. Exploring galactic systems that create dust necessitates a detailed and thorough analysis spanning multiple wavelengths aimed at discerning potential influencers, such as the presence of companion stars. Present endeavors are concentrated on refining data through meticulous telluric line corrections, laying the foundation for subsequent investigations. This iterative process unfolds gradually and methodically, ensuring the maximum smoothness in each graph corresponding to the respective order. Future endeavors aspire to juxtapose observational data with theoretical constructs, emphasizing O stars, thereby enabling more profound insights into the mechanisms governing dust production within these stellar configurations. Ongoing research efforts to clarify the underlying dynamics governing dust production in WR stars, thereby contributing to the comprehension of stellar evolution and interstellar environments.
Probing the Multiplicity of Dusty Wolf-Rayet Stars with Multi-Wavelength Techniques: Survey of Infrared Spectrometry
Wolf-Rayet (WR) stars, emblematic of massive celestial entities in advanced evolutionary phases, wield significant influence over the cosmic background. Carbon-rich WR stars emerge prominently among their ranks, distinguished by their expansive infrared emissions, which foster unique conditions conducive to producing cosmic dust. Exploring galactic systems that create dust necessitates a detailed and thorough analysis spanning multiple wavelengths aimed at discerning potential influencers, such as the presence of companion stars. Present endeavors are concentrated on refining data through meticulous telluric line corrections, laying the foundation for subsequent investigations. This iterative process unfolds gradually and methodically, ensuring the maximum smoothness in each graph corresponding to the respective order. Future endeavors aspire to juxtapose observational data with theoretical constructs, emphasizing O stars, thereby enabling more profound insights into the mechanisms governing dust production within these stellar configurations. Ongoing research efforts to clarify the underlying dynamics governing dust production in WR stars, thereby contributing to the comprehension of stellar evolution and interstellar environments.