Pulsation of M-type Mira variables with moderately different mass: search for observable mass effects
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
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
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