Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...336..527d&link_type=abstract
Astronomy and Astrophysics, v.336, p.527-534 (1998)
Astronomy and Astrophysics
Astrophysics
20
Stars: Binaries: Spectroscopic, Stars: Individual: Theta Tuc, Stars: Oscillations, Stars: Variables: Delta Sct
Scientific paper
Using seven four-hour time series of high-resolution spectra, the binary nature and the oscillations of theta Tuc are investigated. The spectrum is double-lined, proving the binarity. theta Tuc is a binary with a circular orbit and with an anomalous mass ratio q=0.09. The for the first time determined orbital elements are P=7.1036 days, K1=8.6 km/s and K2=95.6 km/s. The oscillations of the delta Scuti-type main component are spectroscopically investigated. Line-profile variations are discovered, and radial-velocity variations reveal a main oscillation frequency of f1=20.27 c/d which corresponds to the main oscillation 20.2806 c/d in photometry. Another frequency, f2=18.82 c/d found in the spectroscopic data and not present in the photometric dataset, needs to be investigated more profoundly. Based on observations collected at the European Southern Observatory, La Silla, Chile. (Observing proposals 57 E-0269 and 58 D-0150)
Daems K.
de Mey K.
Sterken Christiaan
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