Abstract
Beginning in June 2003, undergraduate students and the author have spectroscopically monitored bright Be stars using a custom built fiber-fed spectrograph attached to the UCA Observatory 11-inch Schmidt-Cassegrain telescope. We have obtained 0.8 Angstrom/pixel resolution spectra of the H-alpha line for over forty Be-Stars. Some have been observed on multiple dates in order to detect any temporal changes. Line profiles, velocities, and observed variations for some of these stars will be presented.
Recommended Citation
Austin, Scott
(2004)
"Be Star Spectroscopy Using the UCA Fiber-Fed Spectrograph,"
Journal of the Arkansas Academy of Science: Vol. 58, Article 5.
Available at:
https://scholarworks.uark.edu/jaas/vol58/iss1/5
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