On the Pulsation Mode of Mira Variables: Nonlinear CalculationsCompared with Radii Observations

Details On the Pulsation Mode of Mira Variables: Nonlinear CalculationsCompared with Radii Observations On the Pulsation Mode of Mira Variables: Nonlinear CalculationsCompared with Radii Observations

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...514l..35y&link_type=abstract

The Astrophysical Journal, Volume 514, Issue 1, pp. L35-L37.

Astronomy and Astrophysics

Astronomy

16

Stars: Fundamental Parameters, Stars: Late-Type, Stars: Oscillations

Scientific paper

Observed radii of Mira variables are compared with theoretical nonlinear
calculations. In contrast with previous works, the observed data is
found to be compatible with the fundamental nonlinear mode of pulsation.

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