On the pulsation mode of Mira variables: Nonlinear calculations compared with radii observations

A. Ya'ari*, Y. Tuchman

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

15 Scopus citations

Abstract

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.

Original languageAmerican English
Pages (from-to)L35-L37
JournalAstrophysical Journal
Volume514
Issue number1 PART 2
DOIs
StatePublished - 20 Mar 1999

Keywords

  • Stars: fundamental parameters
  • Stars: late-type
  • Stars: oscillations

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