Astrophysics and Space Science

, Volume 8, Issue 2, pp 262–266 | Cite as

The spectrum of the manganese star ι Coronae Borealis

  • Lawrence H. Aller
  • John E. Ross


Iota Coronae Borealis is a manganese mercury star with a rich spectrum of sharp lines. We tabulate equivalent widths element by element from data obtained at Lick 120-inch telescope.


Mercury Manganese Equivalent Width Sharp Line Rich Spectrum 
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.


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  1. Aller, L. H. and Ross, J. E.: 1967,The Magnetic and Related Stars (ed. by R. C. Cameron), Mono Book Co., Baltimore, p. 339.Google Scholar
  2. Babcock, H. W.: 1958,Astrophys. J. 128, 228.Google Scholar
  3. Bertaud, C.: 1958,J. Observateurs 42, 45.Google Scholar
  4. Bouigue, R.: 1957,Publ. Observ. Haute Provence 4, 52.Google Scholar
  5. Dworetsky, M.: 1969, private communication.Google Scholar
  6. Eggen, O. J.: 1967, inThe Magnetic and Related Stars (ed. by R. C. Cameron), Mono Book Co., Baltimore.Google Scholar
  7. Maestre, L. A. and Deutsch, A. J.: 1961,Astrophys. J. 134, 562.Google Scholar
  8. Osawa, K.: 1959,Astrophys. J. 130, 159.Google Scholar
  9. Ross, J. E. and Aller, L. H.: 1970,Astrophys. J. 161, 189.Google Scholar
  10. Slettebak, A.: 1953,Astrophys. J. 119, 146.Google Scholar

Copyright information

© D. Reidel Publishing Company 1970

Authors and Affiliations

  • Lawrence H. Aller
    • 1
  • John E. Ross
    • 1
  1. 1.University of CaliforniaLos AngelesUSA

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