The inversion of emission line spectra from Wolf-Rayet stars

Details The inversion of emission line spectra from Wolf-Rayet stars The inversion of emission line spectra from Wolf-Rayet stars

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....34..387c&link_type=abstract

Astronomy and Astrophysics, vol. 34, no. 3, Sept. 1974, p. 387-391.

Astronomy and Astrophysics

Astrophysics

5

Atmospheric Models, Emission Spectra, Hot Stars, Line Spectra, Stellar Atmospheres, Stellar Spectra, Wolf-Rayet Stars, Atmospheric Density, Atmospheric Temperature, Mathematical Models, Velocity Distribution

Scientific paper

The investigation reported is concerned with the quantitative estimation of the density, temperature, and velocity distributions on the basis of a direct inversion of the observed emission line spectra. Emission line profiles are computed with the aid of model Wolf-Rayet atmospheres of specified density, temperature, and velocity. The inversion technique is applied to the obtained data and the information content of the emission line in question is examined, taking into account the manner in which the computed distributions converge to the originally specified values.

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