Abstract
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.
Similar content being viewed by others
References
Aller, L. H. and Ross, J. E.: 1967,The Magnetic and Related Stars (ed. by R. C. Cameron), Mono Book Co., Baltimore, p. 339.
Babcock, H. W.: 1958,Astrophys. J. 128, 228.
Bertaud, C.: 1958,J. Observateurs 42, 45.
Bouigue, R.: 1957,Publ. Observ. Haute Provence 4, 52.
Dworetsky, M.: 1969, private communication.
Eggen, O. J.: 1967, inThe Magnetic and Related Stars (ed. by R. C. Cameron), Mono Book Co., Baltimore.
Maestre, L. A. and Deutsch, A. J.: 1961,Astrophys. J. 134, 562.
Osawa, K.: 1959,Astrophys. J. 130, 159.
Ross, J. E. and Aller, L. H.: 1970,Astrophys. J. 161, 189.
Slettebak, A.: 1953,Astrophys. J. 119, 146.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Aller, L.H., Ross, J.E. The spectrum of the manganese star ι Coronae Borealis. Astrophys Space Sci 8, 262–266 (1970). https://doi.org/10.1007/BF00650889
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650889