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Paper: |
Spectroscopic Mode Identification in Slowly-Pulsating Subdwarf B Stars |
Volume: |
392, Hot Subdwarf Stars and Related Objects |
Page: |
253 |
Authors: |
Schoenaers, C.; Lynas-Grey, A.E. |
Abstract: |
Mode identification is crucial for an asteroseismological study of any significance. Contrarily to spectroscopic techniques, methods such as period-fitting and multi-colour photometry do not provide a full reconstruction of non-radial pulsations. We present a new method of spectroscopic mode identification and test it on time-series of synthetic spectra appropriate for pulsating subdwarf-B stars. We then apply it to the newly discovered slowly pulsating subdwarf-B star HD 4539. |
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