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- W71641773 abstract "We have calculated a large number of linear radial pulsation models to fit the periods of AC And. In the parameter regime representative of RR Lyrae stars no models can be found that match the observed periods for any heavy element abundance Z. There are, however, two groups of higher mass models which yield complete agreement between the observed periods and those of the first three radial modes. The first comprises models with 0.001 < Z < 0.002 and masses and luminosities of 1.1 < M/M ○. < 1.4, 100 < L/L ○. < 130 (depending on Z). The second group has higher masses, luminosities and Z, viz. 0.01 < Z < 0.02, M/M ○. ≃ 2.7, 80 < L/L ○. < 200. These ranges are sensitive to the assumed uncertainties of the model periods. We give ranges of model parameters as functions of Z and discuss their uncertainties" @default.
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- W71641773 date "1994-01-01" @default.
- W71641773 modified "2023-09-26" @default.
- W71641773 title "The triple-mode variable AC Andromedae" @default.
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