The Chromosphere/Shock Dilemma of Non-Mira, Late-Type Variable Stars

Details The Chromosphere/Shock Dilemma of Non-Mira, Late-Type Variable Stars The Chromosphere/Shock Dilemma of Non-Mira, Late-Type Variable Stars

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997stin...9892740w&link_type=abstract

Technical Report, NASA/CR-97-112947; NAS 1.26:112947 Educational Inst.

Computer Science

Asymptotic Giant Branch Stars, Models, Chromosphere, Shock Waves, Wave Propagation, Mira Variables, Radiative Transfer, Iue, Variable Stars, Red Giant Stars, Ultraviolet Spectra, Line Spectra, Hydrodynamics

Scientific paper

An investigation of the atmospheric structure of non-Mira, asymptotic giant branch stars through NLTE radiative transfer modeling applied to hydrodynamic models is discussed. Synthetic spectra resulting from these calculations were compared with IUE observations of these stars to test the validity of the models. The development of the hydrodynamic models is detailed.

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