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SALT HRS capabilities for time resolved pulsation analysis: a test with the roAp star α Circini

By D. Holdsworth and Emily Brunsden
Spectroscopy is a powerful tool for detecting variability in the rapidly oscillating Ap (roAp) stars. The technique requires short integrations times and high resolution, and so is limited to only a few telescopes and instruments. To test the capabilities of the High Resolution Spectrograph (HRS) at the Southern African Large... Show more
August 3, 2020
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SALT HRS capabilities for time resolved pulsation analysis: a test with the roAp star $α$ Circini
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