2:1 resonance in RV Tauri stars

Details 2:1 resonance in RV Tauri stars 2:1 resonance in RV Tauri stars

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..125i&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

1

Rv Tauri Stars, 2:1 Resonance, Alternating Minima

Scientific paper

Behavior of two pulsationally unstable modes in 2:1 resonance is examined in relation to the alternating behavior of the deep and shallow minima of the RV Tauri stars. From results obtained from amplitude equations and numerical model calculations, 2:1 resonance seems to be one of the attractive origin of the alternation. Full results will be published elsewhere.

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