Chelen Johnson
Hertzsprung-Russel diagram for Active Galactic Nuclei (HR4AGN): Using space and ground based ultraviolet, optical, and infrared images to find a correlation between the color and luminosity of gas emission and dust emission around supermassive black holes at the centers of galaxies.
One of my students at Niles West had become interested in GRBs as we thought they were the results of mergers of black holes [but we learned this was wrong at an AAS plenary talk]. My student thought it was interesting that scientists could change their minds about how things worked.
I think this [AAS] trip is a crucial part of the program. I learned so much about the many different telescopes, enjoyed the historical presentations, and found the exposure to the more specific research to be beneficial, even if I didn't understand that much about the research itself. It was also a great chance to meet scientists as well as other educators.
This experience has forced me to look at something new and has inspired me to enrich and improve my classes.
