Investigating Classical Be Stars & Their Surrounding Disks

Abstract

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

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