Skip to main content
SpringerLink
Log in

Atmospheric elemental abundances for the components of the multiple system ADS 11061. 41 Draconis

  • Published:
Astronomy Reports Aims and scope Submit manuscript

Abstract

We obtained speckle interferometric and spectroscopic observations of the system 41 Dra during its periastron passage in 2001. The components’ lines are resolved in the spectral interval 3700–9200 Å. The observed wavelength dependence of the brightness difference between the components is used to estimate the B-V indices separately for each of the components: B-V = 0.511 for component a and B-V = 0.502 for component b. We derived improved effective temperatures of the components from their B-V values and hydrogen-line profiles. The observations can be described with the parameters for the components T aeff = 6370 K, log g a = 4.05 and T beff = 6410 K, log g b = 4.20. The iron, carbon, nitrogen, and oxygen abundances in the atmospheres of the components are log N(Fe)a = 7.55, log N(Fe)b = 7.60, log N(C)a = 8.52, log N(C)b = 8.58, log N(N)a = 8.05, log N(N)b = 7.99, log N(O)a = 8.73, log N(O)b = 8.76.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Log in via an institution

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Similar content being viewed by others

References

  1. A. A. Kisilev and L. G. Romanenko, Astron. Zh. 73, 875 (1996) [Astron. Rep. 40, 795 (1996)].

    Google Scholar 

  2. A. Tokovinin, Yu. Yu. Balega, E. A. Pluzhnik, et al., Astron. Astrophys. 409, 245 (2003).

    Article  ADS  Google Scholar 

  3. Yu. Yu. Balega, V. V. Leushin, and G. Weigelt, Bull. Spec. Astrophys. Obs. 54, 5 (2003).

    ADS  Google Scholar 

  4. A. Tokovinin, Pis’ma Astron. Zh. 21, 286 (1995) [Astron. Lett. 21, 250 (1995)].

    ADS  Google Scholar 

  5. I. I. Balega, Yu. Yu. Balega, G. Fal’ke, et al., Pis’ma Astron. Zh. 23, 774 (1997) [Astron. Lett. 23, 172 (1997)].

    Google Scholar 

  6. V. A. Al-Wardat, Yu. Yu. Balega, V. V. Leushin, et al., IAU Symp. No. 210: Modelling of Stellar Atmospheres, June 17–21, 2002, Uppsala, Sweden.

  7. The Hypparcos and Tycho Catalogues. ESA SP-1200, ESA, 1997.

  8. F. A. Musaev, Pis’ma Astron. Zh. 19, 776 (1993) [Astron. Lett. 19, 315 (1993)].

    ADS  Google Scholar 

  9. V. E. Panchuk, I. D. Najdenov, V. G. Klochkova, et al., Bull. Spec. Astrophys. Obs. 44, 127 (1998).

    ADS  Google Scholar 

  10. V. E. Panchuk and S. V. Ermakov, Spets. Astrofiz. Obs., Nauchno-Tekh. Otchet No. 267 (1999).

  11. F. A. Musaev, G. A. Galazutdinov, A. V. Sergeev, et al., Kinematika Fiz. Nebesnykh Tel 15, 282 (1999).

    Google Scholar 

  12. Yu. Yu. Balega, V. V. Leushin, and E. A. Pluzhnik, Bull. Spec. Astrophys. Observ. 51, 61 (2001).

    ADS  Google Scholar 

  13. A. V. Kharitonov, V. M. Tereshchenko, and L. N. Knyazeva, Spectrophotometric Catalogue of Stars (Nauka, Alma-Ata, 1988).

    Google Scholar 

  14. H. L. Johnson and W. W. Morgan, Astrophys. J. 117, 313 (1953).

    ADS  Google Scholar 

  15. V. G. Kornilov, I. M. Volkov, A. I. Zakharov, et al., Catalogue UBVR of Northern Sky Bright Stars (Tr. Gos. Astron. Inst. Shternberga, Moscow, 1991), Vol. 63.

    Google Scholar 

  16. R. Kurucz, http://kurucz.harvard.edu

  17. G. A. Galazutdinov, Preprint No. 92, SAO (Spec. Astrophys. Obs., 1992).

  18. V. V. Tsimbal, Magnetic Stars (Spec. Astrophys. Obs., Russ. Acad. Sci., Nizhnii Arkhyz, 2003) (in press).

    Google Scholar 

  19. V. V. Leushin and G. P. Topil’skaya, Astrofiz. 22, 121 (1985) [Astrophys. 21, 74 (1985)].

    ADS  Google Scholar 

  20. F. Kupka, N. E. Piskunov, T. A. Ryabchikova, et al., Astron. Astrophys., Suppl. Ser. 138, 119 (1999).

    Article  ADS  Google Scholar 

  21. G. Grim, Spectral Line Widening in Plasma (Mir, Moscow, 1978).

    Google Scholar 

  22. N. Grevesse and A. J. Sauval, Solar Composition and Its Evolution—From Core to Corona, Ed. by C. Frolich, M. C. E. Huber, S. K. Solanki, and R. von Steiger (Kluwer, Dordrecht, 1998), p. 161.

    Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Karachai-Cherkessian Republic, 357147, Russia

    Yu. Yu. Balega & V. V. Leushin

  2. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, Bonn, 53121, Germany

    G. Weigelt

Authors
  1. Yu. Yu. Balega
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. V. V. Leushin
    View author publications

    You can also search for this author in PubMed Google Scholar

  3. G. Weigelt
    View author publications

    You can also search for this author in PubMed Google Scholar

Additional information

__________

Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 82, No. 3. 2005, pp. 247–255.

Original Russian Text Copyright © 2005 by Balega, Leushin, Weigelt.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Balega, Y.Y., Leushin, V.V. & Weigelt, G. Atmospheric elemental abundances for the components of the multiple system ADS 11061. 41 Draconis. Astron. Rep. 49, 217–225 (2005). https://doi.org/10.1134/1.1882779

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1134/1.1882779

Keywords

Search

Navigation