The extended atmosphere and evolution of the RV Tauri star, R Scuti

Details The extended atmosphere and evolution of the RV Tauri star, R Scuti The extended atmosphere and evolution of the RV Tauri star, R Scuti

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..107m&link_type=toc

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

Stars: Agb, Stars: Atmospheres, Stars: Individual: R Sct We Found Molecular Bands In Absorption And In Emission In The Infrared Spectra Of The Rv Tau Star, R Sct. This Is A Unique Property Among The Rv Tau Stars, But Rather Commonly Seen In Mira Variables. The Period Evolution Of This Star Does Not Fit With An Ordinary Post-Agb Scenario. Therefore, We Argue An Alternative Choice Of The Evolutional Stage, R Sct Is Not A Post-Agb Star But An Agb Star In The Helium-Burning Phase Of The Thermal-Pulse Cycle.

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