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A&A Supplement Ser., Vol. 124, July 1997, 23-31

Received September 9; accepted October 14, 1996

Nonvariability among tex2html_wrap_inline1017 Bootis stars

E. Paunzen, R. Kuschnig, G. Handler, M. Gelbmann, and W.W. Weiss

Send offprint request: E. Paunzen
Institut für Astronomie der Universität Wien, Türkenschanzstr. 17, A-1180 Wien, Austria


With asteroseismic techniques it is possible to investigate the interior and the evolutionary status of stars via their frequency spectrum. Both information would be very much needed for tex2html_wrap_inline1021Bootis stars, a group of metal-poor PopulationI, A-type stars, since no conclusive theory exists explaining the observed abundance anomalies. Geneva and Strömgren photometry place these stars inside the classical instability strip or at least very close to it. We therefore have started an extensive photometric survey for pulsation in tex2html_wrap_inline1023Bootis stars and have discovered so far 13 new variables.
In this paper we present results for stars which presumably are constant, because we are able to establish only an upper level for possible variability. A typical noise level of 3mmag for Strömgren b was achieved in the relevant frequency domain up to 100dtex2html_wrap_inline1027.
Considering the given noise level of our survey, we conclude that at least 50% of all investigated tex2html_wrap_inline1029Bootis stars inside the instability strip are pulsating, making this group remarkable compared to stars with similar spectral types. This may suggest that a low (surface) metallicity has an influence on the pulsation behavior of stars. New models, as well as further observations are needed to clarify the tex2html_wrap_inline1031Bootis phenomenon using asteroseismic techniques.

keywords: astronomical data bases -- surveys; stars -- tex2html_wrap_inline1033 Bootis; stars -- chemically peculiar; stars -- early type

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