Astronomy and Astrophysics – Astronomy
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sass...30...53g&link_type=abstract
The Society for Astronomical Sciences 30th Annual Symposium on Telescope Science. Held May 24-26, 2011 at Big Bear Lake, CA. Pu
Astronomy and Astrophysics
Astronomy
Scientific paper
Be spectral classification stars typically show variable and complex emission detail in the H alpha spectral line. These emission phenomena are not from the star itself but are thought to originate from a circumstellar disk of material that has formed around the star due to a combination of mass loss, rapid rotation, a magnetically torqued disk of the surrounding material and nonradial stellar pulsation. To analyze these H Alpha line characteristics a high resolution spectrograph is required to display the subtle changes over time. The construction of an inexpensive high resolution Littrow spectrograph for that analysis process is herein described.
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