Pulsation of M-type Mira variables with moderately different mass: search for observable mass effects

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Ireland, Michael
Scholz, M
Tuthill, Peter G
Wood, Peter R

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Blackwell Publishing Ltd

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Models of M-type Miras with masses of 1 and 1.2M⊙, i.e. with envelope masses of about 0.4 and 0.6 M⊙, have been constructed, and a comparison has been made of their observable properties. Geometric pulsation of continuum-forming layers is found to be

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Monthly Notices of the Royal Astronomical Society

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