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Spectral Synthesis of Cool Components of Symbiotic Stars

Published online by Cambridge University Press:  07 August 2017

Claudio B. Pereira  and
Sayd Codina Landaberry
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
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 409 - 410
Copyright
Copyright © Kluwer 1992 

References

References:

Johnson, H. R. and Ake, T. (1989) ‘BD-21.3873: An Heavy Element-Rich Symbiotic?’, Evolution of Peculiar Red Giants Stars. IAU Colloquium, 106.Google Scholar
Jorissen, A. (1989) ‘ER Del : A True Symbiotic S Star?’, Evolution of Peculiar Red Giants Stars. IAU Colloquium, 106.Google Scholar
Little, S. J., Little-Marenin, I. R. and Bauer, W. (1987). ‘Additional Late-Type Stars with Techenetium’, Astron. J. 94,981–995 Google Scholar
Luud, L and Leedyarv, L. (1986). ‘Properties of the Cold Components Of Symbiotic Stars’, Astrophysics, 24, 154–162.Google Scholar
Whitelock, P. A. (1987), ‘Symbiotic Miras’, Publ. Ast. Soc. Pac., 99, 573–591.Google Scholar