Faculty
Faculty of Science
Supervisor Name
Dr. Carol Jones
Keywords
Be Stars, Stars
Description
Identify physical conditions of B-emission stars at certain positions over specific wavelengths. Classify stars based on colors and Identify the spectral type of a star and temperature based on its absorption lines. Summarize the changes and excess in flux over certain wavelengths of multiple B-emission stars while also looking at the flux when filtered over the V, B, U and K bands. Identify properties of the Be stars and evaluate how changing certain properties effect the stars and their surrounding disks.
Acknowledgements
Special thanks to my supervisor Dr. Carol Jones and mentors Dr. Maziar Ghoreyshi and Mark Suffak for their guidance and continued support throughout the study.
This study was supported by the Department of Physics and Astronomy and USRI program of Western University.
Creative Commons License
This work is licensed under a Creative Commons Attribution-Noncommercial 4.0 License
Document Type
Poster
Included in
Investigating Classical Be Stars & Their Surrounding Disks
Identify physical conditions of B-emission stars at certain positions over specific wavelengths. Classify stars based on colors and Identify the spectral type of a star and temperature based on its absorption lines. Summarize the changes and excess in flux over certain wavelengths of multiple B-emission stars while also looking at the flux when filtered over the V, B, U and K bands. Identify properties of the Be stars and evaluate how changing certain properties effect the stars and their surrounding disks.