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Spectral Synthesis of Cool Components of Symbiotic Stars

Published online by Cambridge University Press:  07 August 2017

Claudio B. Pereira
Affiliation:
Observatório Nacional Rua José Cristino, 77 São Cristóvão - CEP 20921 Rio de Janeiro - Brasil
Sayd Codina Landaberry
Affiliation:
Observatório Nacional Rua José Cristino, 77 São Cristóvão - CEP 20921 Rio de Janeiro - Brasil

Abstract

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We analyzed the optical spectra of cool component of symbiotic star SY Mus by means of spectral synthesis technique in order to derive the atomic abundances using the Minneart formulae for computing the atmospheric opacities. We obtained a satisfactory agreement between the observed and computed spectra and the resulting abundances were consistent to the solar abundances.

Type
Near Stellar Environments
Copyright
Copyright © Kluwer 1992 

References

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