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Astrophysics

, Volume 35, Issue 1, pp 340–341 | Cite as

Abundance of palladium group elements in the atmospheres of evolved stars. III. Rhodium

  • M. Ya. Orlov
  • A. V. Shavrina
Brief Communications
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Keywords

Atmosphere Palladium Rhodium Group Element Palladium Group 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Literature Cited

  1. 1.
    M. Ya. Orlov and A. V. Shavrina,Astrofiz.,28, 595 (1988).Google Scholar
  2. 2.
    M. Ya. Orlov and A. V. Shavrina,Astrofiz.,32, 231 (1990).Google Scholar
  3. 3.
    V. F. Gopka and N. S. Komarov,Astron. Zh.,67, 1211 (1990).Google Scholar
  4. 4.
    R. L. Kurucz and E. Peytremann, SAO Spec. Rep. No. 362 (1975).Google Scholar
  5. 5.
    M. Vetesnik,Folia Prirodoved. Fac. UJEP Brno,21, No. 3, 5 (1980).Google Scholar
  6. 6.
    V. V. Smith and D. L. Lambert,Astrophys. J.,294, 326 (1985).Google Scholar
  7. 7.
    S. L. Wright and J. D. Argyros,Comm. Univ. London Observ., No 75, 1 (1975).Google Scholar
  8. 8.
    E. Anders and N. Grevesse,Geochim. Cosmochim. Acta,53, 197 (1989).Google Scholar
  9. 9.
    C. Corliss and W. Boseman,Transition Probabilities and Oscillator Strengths of 70 Elements [Russian translation], Mir, Moscow (1968).Google Scholar
  10. 10.
    É. A. Gurtovenko and R. I. Kostyk,Fraunhofer Spectrum and System of Solar Oscillator Strengths [in Russian], Naukova Dumka, Kiev (1989).Google Scholar

Copyright information

© Plenum Publishing Corporation 1993

Authors and Affiliations

  • M. Ya. Orlov
  • A. V. Shavrina

There are no affiliations available

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