Physics
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992srtoh..12..163t&link_type=abstract
Sci. Rep. Tôhoku Univ., Eighth Ser., Vol. 12, Nos. 2/3, p. 163 - 165
Physics
Scientific paper
The UU Her stars are now believed as pulsating less massive stars. The discovery of double-periodicity for UU Her, once regarded as the type of this group, emphasizes again a serious question on the nature of this star. The period-ratio, the pulsational instability, and the strength of coupling together with the hydrodynamic model will be investigated for UU Her based on new opacities.
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