A differential model atmosphere analysis of the iron spectrum of Epsilon Virginis

Details A differential model atmosphere analysis of the iron spectrum of Epsilon Virginis A differential model atmosphere analysis of the iron spectrum of Epsilon Virginis

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186...85h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 186, Jan. 1979, p. 85-91.

Astronomy and Astrophysics

Astronomy

6

Atmospheric Models, Iron, Red Giant Stars, Stellar Atmospheres, Stellar Models, Line Spectra, Spectrum Analysis, Stellar Gravitation, Stellar Spectra, Stellar Temperature

Scientific paper

A new analysis of the iron abundance in the bright red giant Epsilon Virginis indicates an essentially solar abundance, in good agreement with the abundance reported by Cayrel and Cayrel (1963). The analysis was based on electrographically recorded echelle spectra, and the method of analysis is described. Analysis of the spectroscopic gravity from the collisional damping of the Fe I 5269.55 A wavelength is explained.

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