Multi-wavelength spectroscopy of the stable shell star HD 193182

Details Multi-wavelength spectroscopy of the stable shell star HD 193182 Multi-wavelength spectroscopy of the stable shell star HD 193182

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.208..135d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 208, no. 1, p. 135-151

Astronomy and Astrophysics

Astrophysics

3

Infrared Spectra, Shell Stars, Spectrum Analysis, Ultraviolet Spectra, A Stars, Electron Density (Concentration), Gravitation, Radial Velocity, Temperature

Scientific paper

HD 193182 is one of the most interesting 'stable shell stars' and present stable shell features which seems to be constant over decades. In this research we analyzed optical, ultraviolet and near-infrared spectra of this little-studied shell star. In the meantime we applied model calculations to the measured spectral parameters of HD 193182 in order to present a more complete view of its stellar and envelope characteristics.

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