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- W65634701 abstract "A systematic comparison of observational constraints and theoretical results for the properties of Mira variables is in progress. The observed period-luminosity relation (Feast, M.W., MNRAS, 211, 51P, 1984), the requirement that the mass lie between the core mass (~0.6M⊙) and the main sequence progenitor mass (~1M⊙ at 200 days and ~2M⊙ at 400 days), and the period-mass-radius relation for a given mode suffice to constrain the gross stellar properties L, T and R. In Figure 1 the maximum shock amplitudes are compared with observed velocity amplitudes, assuming Δv/ve = 0.8 for fundamental mode and 0.4 for overtone pulsation (see Willson, this volume)." @default.
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- W65634701 date "1987-01-01" @default.
- W65634701 modified "2023-09-27" @default.
- W65634701 title "A Parameter Study of Terminal AGB Evolution" @default.
- W65634701 doi "https://doi.org/10.1007/978-94-009-3813-7_43" @default.
- W65634701 hasPublicationYear "1987" @default.
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